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		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=102087</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=102087"/>
		<updated>2015-11-02T03:52:38Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Dissertation */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
=Dissertation=&lt;br /&gt;
&lt;br /&gt;
;11/01/2015&lt;br /&gt;
&lt;br /&gt;
Measurements&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:measurements_1.pdf]]&lt;br /&gt;
[[File:measurements_2.pdf]]&lt;br /&gt;
[[File:measurements_3.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Conclusion&lt;br /&gt;
&lt;br /&gt;
[[File:conc.pdf]]&lt;br /&gt;
&lt;br /&gt;
=alpha calibration=&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphaE.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Raw_data_all.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The main peaks are for the following channel numbers,&lt;br /&gt;
&lt;br /&gt;
 You need to redo these plots in publication quality with proper axis labels containing units.&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphap1.png | 150px]]&lt;br /&gt;
[[File:ch_alphap2.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|channel Number|| Energy Upper limit (MeV)|| Energy lower limit (MeV)|| average energy (MeV)||  Notes&lt;br /&gt;
|-&lt;br /&gt;
| 4828 || 4.90 || 4.79 || 4.85 +_ 0.02 ||  &lt;br /&gt;
|-&lt;br /&gt;
| 4869 || 4.94 || 4.83 || 4.88 +_ 0.02 || &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=Gamma Spectrum for U-233=&lt;br /&gt;
&lt;br /&gt;
[[File:gamma_spect.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was before the neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:Meas_conc_1.pdf&amp;diff=102086</id>
		<title>File:Meas conc 1.pdf</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:Meas_conc_1.pdf&amp;diff=102086"/>
		<updated>2015-11-02T03:51:06Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=102085</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=102085"/>
		<updated>2015-11-02T03:47:11Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Dissertation */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
=Dissertation=&lt;br /&gt;
&lt;br /&gt;
;11/01/2015&lt;br /&gt;
&lt;br /&gt;
Measurements&lt;br /&gt;
[[File:measurements_1.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Conclusion&lt;br /&gt;
&lt;br /&gt;
[[File:conc.pdf]]&lt;br /&gt;
&lt;br /&gt;
=alpha calibration=&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphaE.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Raw_data_all.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The main peaks are for the following channel numbers,&lt;br /&gt;
&lt;br /&gt;
 You need to redo these plots in publication quality with proper axis labels containing units.&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphap1.png | 150px]]&lt;br /&gt;
[[File:ch_alphap2.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|channel Number|| Energy Upper limit (MeV)|| Energy lower limit (MeV)|| average energy (MeV)||  Notes&lt;br /&gt;
|-&lt;br /&gt;
| 4828 || 4.90 || 4.79 || 4.85 +_ 0.02 ||  &lt;br /&gt;
|-&lt;br /&gt;
| 4869 || 4.94 || 4.83 || 4.88 +_ 0.02 || &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=Gamma Spectrum for U-233=&lt;br /&gt;
&lt;br /&gt;
[[File:gamma_spect.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was before the neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:Conc.pdf&amp;diff=102084</id>
		<title>File:Conc.pdf</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:Conc.pdf&amp;diff=102084"/>
		<updated>2015-11-02T03:44:25Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=102083</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=102083"/>
		<updated>2015-11-02T03:43:48Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Dissertation */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
=Dissertation=&lt;br /&gt;
&lt;br /&gt;
;11/01/2015&lt;br /&gt;
&lt;br /&gt;
Measurements and conclusion&lt;br /&gt;
&lt;br /&gt;
[[File:conc.pdf]]&lt;br /&gt;
&lt;br /&gt;
=alpha calibration=&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphaE.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Raw_data_all.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The main peaks are for the following channel numbers,&lt;br /&gt;
&lt;br /&gt;
 You need to redo these plots in publication quality with proper axis labels containing units.&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphap1.png | 150px]]&lt;br /&gt;
[[File:ch_alphap2.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|channel Number|| Energy Upper limit (MeV)|| Energy lower limit (MeV)|| average energy (MeV)||  Notes&lt;br /&gt;
|-&lt;br /&gt;
| 4828 || 4.90 || 4.79 || 4.85 +_ 0.02 ||  &lt;br /&gt;
|-&lt;br /&gt;
| 4869 || 4.94 || 4.83 || 4.88 +_ 0.02 || &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=Gamma Spectrum for U-233=&lt;br /&gt;
&lt;br /&gt;
[[File:gamma_spect.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was before the neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=102082</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=102082"/>
		<updated>2015-11-02T03:40:57Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* alpha calibration */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
=Dissertation=&lt;br /&gt;
&lt;br /&gt;
Measurements and conclusion&lt;br /&gt;
&lt;br /&gt;
[[File:meas_conc.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=alpha calibration=&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphaE.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Raw_data_all.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The main peaks are for the following channel numbers,&lt;br /&gt;
&lt;br /&gt;
 You need to redo these plots in publication quality with proper axis labels containing units.&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphap1.png | 150px]]&lt;br /&gt;
[[File:ch_alphap2.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|channel Number|| Energy Upper limit (MeV)|| Energy lower limit (MeV)|| average energy (MeV)||  Notes&lt;br /&gt;
|-&lt;br /&gt;
| 4828 || 4.90 || 4.79 || 4.85 +_ 0.02 ||  &lt;br /&gt;
|-&lt;br /&gt;
| 4869 || 4.94 || 4.83 || 4.88 +_ 0.02 || &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=Gamma Spectrum for U-233=&lt;br /&gt;
&lt;br /&gt;
[[File:gamma_spect.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was before the neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:Gamma_spect.png&amp;diff=101754</id>
		<title>File:Gamma spect.png</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:Gamma_spect.png&amp;diff=101754"/>
		<updated>2015-09-14T23:00:40Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: uploaded a new version of &amp;quot;File:Gamma spect.png&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:Gamma_spect.png&amp;diff=101753</id>
		<title>File:Gamma spect.png</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:Gamma_spect.png&amp;diff=101753"/>
		<updated>2015-09-14T03:09:44Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: uploaded a new version of &amp;quot;File:Gamma spect.png&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:Ch_alphap2.png&amp;diff=101740</id>
		<title>File:Ch alphap2.png</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:Ch_alphap2.png&amp;diff=101740"/>
		<updated>2015-09-11T17:36:47Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:Ch_alphap1.png&amp;diff=101739</id>
		<title>File:Ch alphap1.png</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:Ch_alphap1.png&amp;diff=101739"/>
		<updated>2015-09-11T17:36:29Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101738</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101738"/>
		<updated>2015-09-11T17:36:09Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* alpha calibration */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
=alpha calibration=&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphaE.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Raw_data_all.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The main peaks are for the following channel numbers,&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphap1.png | 150px]]&lt;br /&gt;
[[File:ch_alphap2.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|channel Number|| Energy Upper limit (MeV)|| Energy lower limit (MeV)|| average energy (MeV)||  Notes&lt;br /&gt;
|-&lt;br /&gt;
| 4828 || 4.90 || 4.79 || 4.85 +_ 0.02 ||  &lt;br /&gt;
|-&lt;br /&gt;
| 4869 || 4.94 || 4.83 || 4.88 +_ 0.02 || &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=Gamma Spectrum for U-233=&lt;br /&gt;
&lt;br /&gt;
[[File:gamma_spect.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was before the neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:Gamma_spect.png&amp;diff=101737</id>
		<title>File:Gamma spect.png</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:Gamma_spect.png&amp;diff=101737"/>
		<updated>2015-09-11T17:33:28Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101736</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101736"/>
		<updated>2015-09-11T17:31:58Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* alpha calibration */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
=alpha calibration=&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphaE.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Raw_data_all.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The main peaks are for the following channel numbers,&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|channel Number|| Energy Upper limit (MeV)|| Energy lower limit (MeV)|| average energy (MeV)||  Notes&lt;br /&gt;
|-&lt;br /&gt;
| 4828 || 4.90 || 4.79 || 4.85 +_ 0.02 ||  &lt;br /&gt;
|-&lt;br /&gt;
| 4869 || 4.94 || 4.83 || 4.88 +_ 0.02 || &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Gamma Spectrum for U-233=&lt;br /&gt;
&lt;br /&gt;
[[File:gamma_spect.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was before the neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:Ch_alphaE.png&amp;diff=101735</id>
		<title>File:Ch alphaE.png</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:Ch_alphaE.png&amp;diff=101735"/>
		<updated>2015-09-11T17:21:50Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: uploaded a new version of &amp;quot;File:Ch alphaE.png&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101704</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101704"/>
		<updated>2015-09-08T17:46:45Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* alpha calibration */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
=alpha calibration=&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphaE.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Raw_data_all.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The main peaks are for the following channel numbers,&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|channel Number|| Energy Upper limit (MeV)|| Energy lower limit (MeV)|| average energy (MeV)||  Notes&lt;br /&gt;
|-&lt;br /&gt;
| 4828 || 5.08 || 5.00 || 5.04 ||  &lt;br /&gt;
|-&lt;br /&gt;
| 4869 || 5.12 || 5.042 || 5.27 || &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was before the neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:Ch_alphaE.png&amp;diff=101703</id>
		<title>File:Ch alphaE.png</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:Ch_alphaE.png&amp;diff=101703"/>
		<updated>2015-09-08T17:32:50Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: uploaded a new version of &amp;quot;File:Ch alphaE.png&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101663</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101663"/>
		<updated>2015-09-03T17:07:28Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* alpha calibration */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
=alpha calibration=&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphaE.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Raw_data_all.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The main peaks are for the following channel numbers,&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|channel Number|| Energy Upper limit || Energy lower limit || average energy ||  Notes&lt;br /&gt;
|-&lt;br /&gt;
| 4828 || 5.25&lt;br /&gt;
|-&lt;br /&gt;
| 4869 || &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was before the neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101662</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101662"/>
		<updated>2015-09-03T16:55:40Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* alpha calibration */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
=alpha calibration=&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphaE.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Raw_data_all.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The main peaks are for the following channel numbers,&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|channel Number|| Energy Upper limit || Energy lower limit || average energy ||  Notes&lt;br /&gt;
|-&lt;br /&gt;
| 4828 || &lt;br /&gt;
|-&lt;br /&gt;
| 4869 || &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was before the neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101661</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101661"/>
		<updated>2015-09-03T16:50:49Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* alpha calibration */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
=alpha calibration=&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphaE.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Raw_data_all.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The main peaks are for the following channel numbers,&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was before the neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:Raw_data_all.pdf&amp;diff=101638</id>
		<title>File:Raw data all.pdf</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:Raw_data_all.pdf&amp;diff=101638"/>
		<updated>2015-09-01T22:18:00Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:Ch_alphaE.png&amp;diff=101637</id>
		<title>File:Ch alphaE.png</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:Ch_alphaE.png&amp;diff=101637"/>
		<updated>2015-09-01T22:17:37Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101636</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101636"/>
		<updated>2015-09-01T22:17:10Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
=alpha calibration=&lt;br /&gt;
&lt;br /&gt;
[[File:ch_alphaE.png | 150px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Raw_data_all.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was before the neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Ideas&amp;diff=101501</id>
		<title>Ideas</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Ideas&amp;diff=101501"/>
		<updated>2015-08-25T14:07:31Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Will we be able to change the distance between the cards electrically or manually without opening the chamber to avoid disturbing the detection environment???.&lt;br /&gt;
&lt;br /&gt;
[[File:little_better.png| 250px]]&lt;br /&gt;
&lt;br /&gt;
Will a jack be good idea in this case???&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Gaseous_Medium_Physical_Concepts&amp;diff=101204</id>
		<title>Gaseous Medium Physical Concepts</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Gaseous_Medium_Physical_Concepts&amp;diff=101204"/>
		<updated>2015-06-23T14:54:38Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Diffusion */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Related Physical Concepts=&lt;br /&gt;
&lt;br /&gt;
The gaseous medium inside a detector's chamber contains different physical processes as a particle arrives the gas. When the desired particles penetrate the gaseous medium, they directly or indirectly (neutron '''''fission''''')  '''''ionize''''' the gas. If the event happened in the active detection area of the detector, a drift '''''electric field''''' guides the primary and secondary electrons toward the GEM preamplifiers, These preamplifiers are placed to have a separation distance within a limit to not lose the electrons by keeping their '''''diffusion''''' to be a reason for their '''''multiplication''''' . An electron  avalanches appear and the negative voltage directs them toward the read out plate which collects the electrons to show them as negative pulses on the oscilloscope's screen. Electron '''''recombination''''', '''''deattachment''''' and '''''capture'''''  take place in every stage in the electron trip before they reach the readout plate. The output signal is important to measure the detector's performance by determining its efficiency, dead time, gain, spatial resolution and robustness.Theoretically, the detector output can be evaluated by solving Boltzmann equation that considers the effect of each physical process occurred.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Ionization==&lt;br /&gt;
&lt;br /&gt;
Ionization is the liberation of an electron from the medium's atoms or its molecules. The minimum amount of energy required to liberate the electron is referred to as the ionization energy.  When the ionizing particle gets in the medium, it deposits its energy to scatter free electrons which they get their kinetic energy after losing part of their energy in releasing from the atom confinement, and after passing through electron-electron collisions. For instance, charged particles like fission fragments ionizes the medium and scatter free electrons, the kinetic energy depends on the fission fragment's energy gained after ionization and the number of collisions the electron passes through. &lt;br /&gt;
&lt;br /&gt;
The ionization is a stochastic process, it depends on the ionization cross section that is determined by the ionizing particle energy, and mass(heavy or light in case of fission fragments). However, the amount of energy needed to have an ionization event on average is the same, regardless of the incident particle type or energy as shown in the following table for argon gas.&amp;lt;ref name=&amp;quot;Veenhof&amp;quot;&amp;gt; R. Veenhof, Internal Note/TPC, ALICE-INT-2003-29 version 1.0, 2003&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Type of particle and its energy || 9 keV x-rays || 10 keV electrons || 40 keV electrons || x-rays Ar-37(K-capture)(5-25 keV) + beta ||alpha 7.68 MeV || 340 MeV protons &lt;br /&gt;
|-&lt;br /&gt;
|Energy per ion-electron pair (eV) || 27.9 &amp;lt;math&amp;gt;\pm&amp;lt;/math&amp;gt; 1.5 ||    27.3            || 25.4    ||  27.0 &amp;lt;math&amp;gt;\pm&amp;lt;/math&amp;gt;0.5 || 26.25 || 25.5&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Ionization in fission chambers===&lt;br /&gt;
&lt;br /&gt;
Ionization by a fission fragment is not  the only source for free electrons and it  is not the only ionization process in fission chamber. Fission chambers usually contain  neutoron fissinable materials, they are heavy radioisotopes that decay and emit more than one type of the ionizing radiation or  by their daughters after decay. For instance, when the fission chamber contains U-233, free electrons are detected because of escaping fission fragments, alpha particles, beta particles, or gamma rays. More specific details about U-233 decay products is shown by the following tables:&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
To count the free electrons produced by the fission fragments demands some modifications in the detector design which mentioned in details in detector construction section .&lt;br /&gt;
&lt;br /&gt;
They are other  physical processes occur in the medium which are related to the gas mixture properties such as: photoionization, thermal ionization, deionization by attachment (negative ion formation) , photoelectric emission, electron emission by excited atoms or positive ion,penning ,and field emission &amp;lt;ref name=&amp;quot;Kuffel&amp;quot;/&amp;gt;. The previous processes may share in decreasing or increasing the number of free electrons in the medium, so evaluating the number of free electrons before preamplification becomes sophisticated without a computer simulation.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Garfield simulates the ionization in the gas mixture cosidering all the former physical processes, it has the ability to simulate the electrons multiplication by GEM preaplifiers, it accepts external solutions for the electric field by other software packages like ANSYS, and it has more than one package such as  Magboltz, HEED, and  Imonte 4.5 that can be used for more precise simulations &amp;lt;ref name=&amp;quot;Veenhof&amp;quot;/&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=Diffusion=&lt;br /&gt;
&lt;br /&gt;
;Main differences between electrons and ions behavior in a gas &amp;lt;ref name=&amp;quot;Mason&amp;quot;&amp;gt;Mason, Edward A. and Earl W. MacDaniel. 1988. Transport Properties of Ions in Gases. John Wiley &amp;amp; Sons. QC717.5 I6 M37 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Studying diffusion and mobility  of  charged particles in a gas is classified in to two main groups, ion and electron diffusion and mobility. They are conceptually similar, but they have many differences. First, The ratio between the mass of the electrons and the gas atoms is very small, so with a few eV work done by the electric field, the electrons will gain a high velocity compared to that of the ions that are accelerated under the same electric field. Also, the probability of low energy electrons to make an interaction is higher than that of the low energy ions, the electron interactions are a supported with accurate calculations for the electron drift velocity. Electrons at low energy have the ability to produce vibrations and excitations in the gas atoms or molecules which are measured within the lab frame, but low energy ions have very low cross sections for most of the interactions with a gas atoms or molecules. When interactions happen, a complexity appears in measuring the ion interactions' products, but the calculations are simpler for  the velocity distribution for the electrons in many gases, since the ratio between a gas atom or molecule mass to the electron mass is very small. Since Producing electrons is simpler than producing ions in a gas,  many interactions are responsible for producing electrons, such as thermionic emission, photoemission, or radioactive decay. On the other hand,  creating an ion requires electron bombardment, photo-ionization or an electric discharge which requires more sophisticated conditions for the experiment and they are not as sensitive as the electrons for the the non-uniformity of the electric field, electric potential and magnetic field. Finally, the existence of the impurities is always a concern; the ions lose most of their energy in the molecular level, but the electron energy loss  within the atomic level in a pure gas, as a result, the ionic velocity distribution is not affected by the existence of these impurities except for some cases related to a highly accurate ionic studies in gases.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electron Diffusion==&lt;br /&gt;
&lt;br /&gt;
[[Diffusion]]&lt;br /&gt;
&lt;br /&gt;
==ion Diffusion==&lt;br /&gt;
&lt;br /&gt;
[[Ion Diffusion]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Multiplication ==&lt;br /&gt;
&lt;br /&gt;
[[GEM pre-amplification]]&lt;br /&gt;
&lt;br /&gt;
==Decreasing the discharge in THGEM==&lt;br /&gt;
&lt;br /&gt;
GEm and THEGM preamplifiers are designed to be rebust, economical, and to get the maximum gain with the least discharge effect. &lt;br /&gt;
&lt;br /&gt;
The discharge effect is when you experimentally start observing sparks coming from the detector. Whenever discharge becomes phenomenon to study then the probability of discharge is used. The probability of discharge is defined as the ratio between the observed frequency of the breakdown and source rate &amp;lt;ref name=&amp;quot;bachmann&amp;quot;/&amp;gt;.The discharge rate and the source rate can be represented as function of position as shown in the figure. &lt;br /&gt;
&lt;br /&gt;
                              &lt;br /&gt;
[[Image:sourcerate_dischargerate_position_bachmann.png |thumb| Fig. Discharge rate and the detected source rate can be represented as function of position &amp;lt;ref name=&amp;quot;bachmann&amp;quot;/&amp;gt;]]&lt;br /&gt;
&lt;br /&gt;
Producing these sparks refers to many reasons,it is obviously observed  when a highly ionizing ion passes through the gaseous chamber and produces enough free electrons to break down the rigidity of surrounding gas by having an avalanche size exceeds Raether limit ( &amp;lt;math&amp;gt; 10^7&amp;lt;/math&amp;gt; electron-ion pairs) when separating the electrodes vertically with small a distance &amp;lt;ref name=&amp;quot;bachmann&amp;quot;&amp;gt; Bachmann et al NIM A 479 (2002) 294-308 &amp;lt;/ref &amp;gt; .&lt;br /&gt;
&lt;br /&gt;
Temperature, humidity, and gas flow externally affect the probability of the transition from the proportional multiplication to a discharge at a given potential, the effect clearly appears in absence of the amplification internal effects as the design quality and the history of the electrodes &amp;lt;ref name=&amp;quot;bachmann&amp;quot;/&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
In case of heavily ionizing ions like alpha particles, an increase in gain causes the probability of discharge to increase, but the increment in the probability of discharge can be decreased by choosing an appropriate gap between the THGEM cards &amp;lt;ref name=&amp;quot;bachmann&amp;quot;/&amp;gt;. As a result, achieving a maximum gain for an incident particle on a chamber with a specific gas mixture ,under a  voltage applied on the THGEM cards, requires an appropriate distance that increases with increment of the ionization rate, i.e an alpha particle requires a bigger gap between the THGEM cards than that of a gamma ray to avoid the discharge effect.(can be experimentally proven). &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:Discharge_probability_gain_doubleGEM_bachmann.png |thumb| Fig. Discharge probability as function of gain for double GEM detector &amp;lt;ref name=&amp;quot;bachmann&amp;quot;/&amp;gt;]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Experimetally, GEM and THGEM have similarities in factors that increases discharge in radiation harsh environment. Being  charge preamplifiers requires a high voltage provided by a voltage divider network which does not have resistors of order of hundred Mohm. Setting the power supply to the maximum current limit causes a discharge,indeed high network resistors up to hundreds of Mohm may limit the effect fo the returning current which will casue less discharge in the GEM or THGEM. Generally, the HV-circuit divides the voltage for triple GEM based detector in away that the voltage difference between the top and bottom of of the first preamplifer is 10% more than the second, and the second preamplifer is 10% more in voltagethan the third one to avoid the discharge effect throught the detector operaion.&lt;br /&gt;
&lt;br /&gt;
The discharge probability is independent on gap voltage between two successive preamplifiers but adding 50 pF capacitor &amp;quot;lower the threshold considerably to the charge propagation&amp;quot;. The charge propagation relies on the capacitance of GEM. Having the GEM with independently powered sectors reduces &amp;quot;the probability of energetic discharge propagation to the readout plate. &lt;br /&gt;
&lt;br /&gt;
In some gases, The highest gain value ,in presence of heavily ionizing radiation, is affected by the gap between the THGEM cards due to the photon feedback mechanics.&amp;lt;ref name=&amp;quot;Bachmann&amp;quot;&amp;gt; Nucl. Inst. and meth. 479 (2002) 294-308 &amp;lt;/ref&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Photon feedback: emission and re-absorption of the photons in the gas or in the metal's surface.&lt;br /&gt;
&lt;br /&gt;
=Reminders=&lt;br /&gt;
&lt;br /&gt;
;Basic definitions&amp;lt;ref name=&amp;quot;Petrovic&amp;quot;&amp;gt; Z Lj Petrovi´c, S Dujko J. Phys. D: Appl. Phys. 42 (2009) 194002 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
1- Enhanced electron conductivity: effect shows an increase in the electron drift velocity in a system encounters inelastic collisions with small probability for drift velocity in all directions when it is directed by an electric field.&lt;br /&gt;
&lt;br /&gt;
2- Negative differential conductivity: An effect is observed when the increase in  electric field density ratio leads to a decrease in the drift velocity. &amp;quot;NDC was found to be favoured by increasing momentum transfer and decreasing inelastic cross sections and the balance of different processes affecting it can be put into a condition which is relatively accurate&amp;quot;. it observed in argon mixtures.&lt;br /&gt;
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;Physical parameter and its eefect on the detector properties&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|physical parameter || Effect on the detector properties &amp;lt;ref name=&amp;quot;Veenhof&amp;quot;/&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
||Electron drift velocity || Dead time&lt;br /&gt;
|-&lt;br /&gt;
| Electron transverse diffusion || Spatial resolution (momentum resolution), transverse resolution should match the response function (signal width)&lt;br /&gt;
|-&lt;br /&gt;
| Townsend Coefficient || Gain which improves the resolution&lt;br /&gt;
|-&lt;br /&gt;
|Attachment Coefficient || Losing the information about an ionization, affects the position information and dE/dx identification &lt;br /&gt;
|-&lt;br /&gt;
|Gas breakdown || Discharge at that voltage&lt;br /&gt;
|-&lt;br /&gt;
| Ion mobility || Determine the rate of collecting the electrons (if the space charge is eliminated), the signal duration in the readout plate&lt;br /&gt;
|-&lt;br /&gt;
|Ionization rate || Affect the spatial resolution, dE/dx identification&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=Boundary Element Method (BEM)=&lt;br /&gt;
&lt;br /&gt;
Boundary Element Method is used to solve Laplace or Poisson Equation, a function u(x,y,z) is solved on the domain boundary and the function partial derivatives are evaluated by integrating on the number of elements on the boundary.&amp;lt;ref name=&amp;quot;Kuffel&amp;quot;&amp;gt;  Kuffel, W. S. Zaengl, J. Kuffel, High voltage engineering: fundamentals, Biddle Ltd, 2nd edition, 2000 &amp;lt;/ref&amp;gt;.&lt;br /&gt;
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GO BACK [https://wiki.iac.isu.edu/index.php/Performance_of_THGEM_as_a_Neutron_Detector]&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=HM_2014&amp;diff=101202</id>
		<title>HM 2014</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=HM_2014&amp;diff=101202"/>
		<updated>2015-06-17T21:10:42Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Iac data Thu. 03/26 */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Iac data Thu. 03/26=&lt;br /&gt;
Cath. V=3.5 kV&lt;br /&gt;
GEM V=2.8 kV&lt;br /&gt;
&lt;br /&gt;
8851 qdc channel 4, TDC 23 before run8859 switch to 29 , PDC 13.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
runs expected to have good in info :8850 8858&lt;br /&gt;
8875, 8876,&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
shutter closed: 8877 (without target).8878&lt;br /&gt;
&lt;br /&gt;
[[ IAC data analysis for GEM ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was before the neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=GEM Gain=&lt;br /&gt;
&lt;br /&gt;
Garfield simulated the ref. gain of triple GEM. Garfield simulated the triple GEM gain in Ar/CO2 93/7, the following figure shows the results of studying of gain as funtion of each GEM voltage.&lt;br /&gt;
&lt;br /&gt;
[[File:ref_data_gain_triple_Ar93_CO2.png |300px]]&lt;br /&gt;
&lt;br /&gt;
the measurement are all within one standard deviation for all the points, so garfield is able to simulate the gain for Ar/CO2 90/10 that we used for our detector within one standard deviation.&lt;br /&gt;
&lt;br /&gt;
=Peak shift measurements for ADC=&lt;br /&gt;
&lt;br /&gt;
filter Amp. x2. int. 500 ns , attenuator 1 dB.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|cath (kV)|| V_drift ||  V_GEM (kV) || open || closed || notes&lt;br /&gt;
|-&lt;br /&gt;
| 3.5 || 700 || 2.8  || 8655 || 8656 || 5 min. for all&lt;br /&gt;
|-&lt;br /&gt;
| 3.5 || 700 || 2.8  || 8657 || 8658 || &lt;br /&gt;
|-&lt;br /&gt;
| 3.5 || 700 || 2.8  || 8659 || 8660 || &lt;br /&gt;
|-&lt;br /&gt;
| 3.5 || 700 || 2.8  || 8661 || 8662 || &lt;br /&gt;
|-&lt;br /&gt;
| 3.5 || 700 || 2.8  || 8663 || 8664 || &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[File: ave_QDC_charge_2.8_3.5kV.png|| 300px]]&lt;br /&gt;
&lt;br /&gt;
filter Amp. x2. int. 500 ns , attenuator 2 dB.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|cath (kV)|| V_drift ||  V_GEM (kV) || open || closed || notes&lt;br /&gt;
|-&lt;br /&gt;
| 3.6 || 700 || 2.9  || 8667 || 8668 || 5 min. for all&lt;br /&gt;
|-&lt;br /&gt;
| 3.6 || 700 || 2.9  || 8669 || 8670 || &lt;br /&gt;
|-&lt;br /&gt;
| 3.6 || 700 || 2.9  || 8671 || 8672 || &lt;br /&gt;
|-&lt;br /&gt;
| 3.6 || 700 || 2.9  || 8673 || 8674 || &lt;br /&gt;
|-&lt;br /&gt;
| 3.6 || 700 || 2.9  || 8675 || 8676 || open and source 8677 (7min.)&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[File:ave_QDC_charge_2.9_3.6kV.png|| 300px]]&lt;br /&gt;
&lt;br /&gt;
filter Amp. x2. int. 500 ns , attenuator 4 dB.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|cath (kV)|| V_drift ||  V_GEM (kV) || open || closed || notes&lt;br /&gt;
|-&lt;br /&gt;
| 3.7 || 700 || 3.0  || 8680 || 8681 || 5 min. for all source on 8683, 8682(7min.)&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The same setting another two runs for shutter open source off and when source is on for an hour: &lt;br /&gt;
&lt;br /&gt;
source off : 8684 for 5 min. (surprisingly ADC is overcharged&lt;br /&gt;
&lt;br /&gt;
source off : 8685 for 5 min. with 5 dB.&lt;br /&gt;
source on : 8686 1h.&lt;br /&gt;
&lt;br /&gt;
[[File:sourceon_off_3kG_3.7C.png || 300px]]&lt;br /&gt;
[[File:PADC_sourceon_off_3kG_3.7C.png || 300px]]&lt;br /&gt;
&lt;br /&gt;
As the source is on the detector, the ADC or PADC did not show any difference compared to the one as the source is off.&lt;br /&gt;
&lt;br /&gt;
=Beta Primary and Secondary Ionization =&lt;br /&gt;
&lt;br /&gt;
U-233 Beta particles are another source of ionization in Ar/CO2 gas. U-233 source emits negative beta particles in wide range of energy,&lt;br /&gt;
&lt;br /&gt;
[[File: beta_energy_percentages.png  | 300 px]]&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
but mostly the energy of emitted beta is in the range 9-20 keV. in the former energy range the yield is in between 0.1-1 percent as shown in the figure above.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Beta's Primary and Secondary Ionization &lt;br /&gt;
&lt;br /&gt;
When a beta particle travels in Ar/CO2 gas, it ionizes the gas which produce primary and secondary electrons. Ar/Co2 gas mixture is used for detecting beta particles, When beta particles travel through the medium, they mostly collide with the medium atoms to ionize the atoms, or to excite the atoms. For instance,  When a 100 keV beta travels in pure argon gas, it produces primarily  1000 ip/cm and 3000 ip/cm secondaries. &amp;lt;ref&amp;gt; Fabio, S. (2014). Basic processes in gaseous counters. In Gaseous Radiation Detectors: Fundamentals and Applications. Cambridge: University Printing House &amp;lt;/ref&amp;gt; &lt;br /&gt;
G4 simulated 100keV beta particle in pure argon gas,and evaluated the number of primary and secondary electrons produced in a 1 cm of  pure Ar gas, the result showed that G4  counted for 906 ip/cm as primaries, and 3455 ip/cm as secondaries, which was within 10 percent for number of expected primaries, and was within 15 percent for the number of secondaries in pure argon. So G4's example would predict the primary and secondary ionization for other beta energies within almost the same errors as shown in the figure below,&lt;br /&gt;
&lt;br /&gt;
[[File: G4_1cmAr90CO2_Beta_primaryElecN.png| 300 px]]&lt;br /&gt;
[[File: G4_1cmAr90CO2_alpha_SecondElecN.png| 300 px]]&lt;br /&gt;
&lt;br /&gt;
which showed that the number of primary and secondary electrons decreased as the incident beta energy increased, also it showed that when the incident beta energy is more that 200keV, the change in the number of primary and secondary electrons became almost negligible.&lt;br /&gt;
&lt;br /&gt;
G4 helped in understanding the effect of adding the shutter in the drift region on Beta's ionization. U-233 emits beta particles in range reaches to 600 keV, and as low as 5 keV in different percentages, which made the shutter affect the number of electrons that ionization produced. According to G4 simulation, the shutter has the ability to stop beta particles of an energy reaches 600 keV and the transmission ration is below 15% as shown in the figure below,&lt;br /&gt;
&lt;br /&gt;
[[File:G4_e_tran_FR4_Ar90.png| 300 px]]&lt;br /&gt;
&lt;br /&gt;
in addition to the fact the emission percentages for higher than 400 keV beta particles is below 0.001 percent, so the shutter stops all beta particles that may travel through the drift region.&lt;br /&gt;
&lt;br /&gt;
As the shutter is open, the highest percentage for beta particles that has energy of 10-40 keV which will make the amount of the produced charge from ionization to be,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; charge = 1.6 \times 10^{-19} C/e^- \times 389 \times 7.88 \times 10^3 = 4.9 \times 10^{-13} = 0.49 pC &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; charge = 1.6 \times 10^{-19} C/e^- \times 1180 \times 7.88 \times 10^3= 1.48 \times 10^{-12} = 1.48 pC &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
for 10keV and 40 keV successively after preamplification.&lt;br /&gt;
&lt;br /&gt;
=G4 and Sauli=&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Particle || Primary || Secondary&lt;br /&gt;
|-&lt;br /&gt;
| 1 keV X-ray || 0.69 ||  72&lt;br /&gt;
|-&lt;br /&gt;
| 100keV electron || 906 ip/cm|| 3455 ip/cm&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
which make the simulation close up to 10% for the primary and secondary electrons.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Particle || Primary || Secondary&lt;br /&gt;
|-&lt;br /&gt;
| 1 keV X-ray || 1 || 50 &lt;br /&gt;
|-&lt;br /&gt;
| 100keV electron || 1000 ip/cm|| 3000 ip/cm&lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV alpha particle || 10^4 || 3X10^4&lt;br /&gt;
|} &lt;br /&gt;
Fabio Sauli, Gaseous Radiation Detectors: Fundamentals and Applications. &lt;br /&gt;
[https://books.google.com/books?id=ToaYAwAAQBAJ&amp;amp;pg=PA20&amp;amp;lpg=PA20&amp;amp;dq=%22argon+gas%22+and+ionization+and+%22primary+electrons%22&amp;amp;source=bl&amp;amp;ots=S1s3U6ImJP&amp;amp;sig=8gt4zvbYGYSxPOHInDNQ-i910es&amp;amp;hl=en&amp;amp;sa=X&amp;amp;ei=NwPrVIPONM_woAT2h4DYDg&amp;amp;ved=0CCkQ6AEwAg#v=onepage&amp;amp;q=%22argon%20gas%22%20and%20ionization%20and%20%22primary%20electrons%22&amp;amp;f=false] page 21.&lt;br /&gt;
&lt;br /&gt;
=02/17/15 QDC &amp;amp; PS-ADC measurements=&lt;br /&gt;
each run lasted for 5 min. unless is mentioned differently&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|cath (kV)|| V_drift ||  V_GEM (kV) || open || closed || notes&lt;br /&gt;
|-&lt;br /&gt;
| 3.87 || 1000 || 2.87 || 8569 || 6570 || &lt;br /&gt;
|-&lt;br /&gt;
| 3.57 || 700 ||  2.87 || 8572|| 8571 || QDC does not show a observed difference between open and closed shutter&lt;br /&gt;
|-&lt;br /&gt;
| 3.57 || 700 ||  2.87 || 8573|| 8574 ||&lt;br /&gt;
|-&lt;br /&gt;
| 3.87 || 1000 || 2.87 || 8576 || 6575 || &lt;br /&gt;
|-&lt;br /&gt;
| 3.87 || 1000 || 2.87 || 8578 || 6577 || &lt;br /&gt;
|-&lt;br /&gt;
| 3.87 || 1000 || 2.87 || 8580 || 6579 || &lt;br /&gt;
|-&lt;br /&gt;
| 3.87 || 1000 || 2.87 || 8582 || 6581 || &lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;QDC Calibration &lt;br /&gt;
&lt;br /&gt;
A triangle test pulse was ejected into the QDC for calibration, details of the pulse amplitude (mV) and width (us) in the table below&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| amplitude (mV) +_ 0.10 || width (us) +_0.10  || charge (nC)   || channel number || run number&lt;br /&gt;
|-&lt;br /&gt;
| 2.04 || 1.56|| 0.03 +_ 0.13|| 1513.2 +_ 1.8 || 8591&lt;br /&gt;
|-&lt;br /&gt;
| 7.00 || 2.32 ||0.16 +_ 0.37 || 2161.7 +_ 1.5 || 8589&lt;br /&gt;
|-&lt;br /&gt;
|10.00 || 2.46 || 0.25 +_ 0.51|| 2767.5 +_ 1.5 || 8592&lt;br /&gt;
|-&lt;br /&gt;
| 13.00 || 2.64 || 0.34 +_ 0.66|| 3169.7 +_ 1.2 || 8593&lt;br /&gt;
|-&lt;br /&gt;
| 17.50 || 2.65 || 0.46 +_ 0.89|| 3618.2 +_ 0.9 || 8585 &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;  charge = 0.5*\left ( \frac {2.04 mV *1.56 \mu s}{50 \Omega}\right ) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:QDC_cal_02_19_15.png | 200px ]]&lt;br /&gt;
&lt;br /&gt;
;QDC Calibration &lt;br /&gt;
&lt;br /&gt;
Asqaure test pulse was ejected into the QDC for calibration, details of the pulse amplitude (mV) and width (us) in the table below&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| amplitude (mV) +_ 0.10 ||  charge (nC)   || channel number || run number&lt;br /&gt;
|-&lt;br /&gt;
| 7.00 ||1.14  ||  407.3+_ 0.5 || 8617&lt;br /&gt;
|-&lt;br /&gt;
| 8.00 || 1.30 || 1077.0 +_ 0.002 || 8618&lt;br /&gt;
|-&lt;br /&gt;
|9.00 || 1.47 || 2210.3 +_ 0.4||  8619&lt;br /&gt;
|-&lt;br /&gt;
| 10.00 || 1.63|| 3422.0 +_ 0.4|| 8620&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
pulse width was 8.16 us. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;  charge = \left ( \frac {1.14 mV *8.16 \mu s}{50 \Omega}\right ) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:QDC_cal_02_22_15.png | 200px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The after signal processing of an input signal of 11.2 mV,the QDC's input signal is 20.8 mV according to what observed on the oscilloscope.&lt;br /&gt;
&lt;br /&gt;
Roy's measurements is as the following &lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; celdetectorV&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Depending on G4 simulation, each alpha particle has 270k secondary electrons which appear as a result of ionization.&lt;br /&gt;
their total charge is &lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; charge =\left (  2.7\times 10^5 \mbox {e}^-\right ) \left (1.6 \times* 10^{-19}  \frac{\mbox{Coul}}{\mbox{e}^-}\right )= 4.32 \times 10^{-14} C   = 43.2  pC &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
 why is the charge multiplied by 2?&lt;br /&gt;
&lt;br /&gt;
 you need to document the amplification of this charge to describe how it is measured by ADC. &lt;br /&gt;
&lt;br /&gt;
Compared to the measured charge spectrum, the figure below average spectrum of five different measurements after subtracting the pedestal.&lt;br /&gt;
&lt;br /&gt;
[[File:QDC_charge_2.87_3.87kV_02_17_15.png| 200px ]]&lt;br /&gt;
&lt;br /&gt;
=1/15/15=&lt;br /&gt;
&lt;br /&gt;
#Rate calculation (Shutter Open)&lt;br /&gt;
&lt;br /&gt;
[https://wiki.iac.isu.edu/index.php/Beta_Transmission_and_Ionization#Combined_Gamma_Emission]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
#SNR -vs- &amp;lt;math&amp;gt;\Delta&amp;lt;/math&amp;gt; V&lt;br /&gt;
&lt;br /&gt;
=01/11/15  2.97kV GEM =&lt;br /&gt;
&lt;br /&gt;
[[cathode drift potential and count rate runs for 2.97kV GEM]]&lt;br /&gt;
&lt;br /&gt;
[[cathode drift 1-1.1k potential and count rate runs for 2.87kV GEM]]&lt;br /&gt;
&lt;br /&gt;
=01/08/14 Peak shift with changing the GEM preamp. Voltage=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The ratio of signal to noise for each voltage is show below:&lt;br /&gt;
&lt;br /&gt;
[[File:2.6-9_sig_noi_ratio.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: 2.6-9_sig_noi_ratio_open_closed_sub.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Even if the error bars looks small in the first figure that shows the sig./noi. and voltage of the GEM, it is noticed the error bars insect for the measurements of open shutter and the open-closed. So the error bars of the first figure can't tell if the increment of 100V for the GEM preamp's is really causing a change in the collected charge spectra.&lt;br /&gt;
&lt;br /&gt;
=12/31/14 Peak shift with changing the GEM preamp. Voltage=&lt;br /&gt;
&lt;br /&gt;
The following figures show the effect of opening and closing the shutter as the GEM voltage is 2.67, 2.87 and 2.97 kV.&lt;br /&gt;
&lt;br /&gt;
[[File:GEM2.6-9_open.png | 300px]]&lt;br /&gt;
[[File:GEM2.6-9_closed.png | 300px]]&lt;br /&gt;
[[File:GEM2.6-9_sub.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
The ratio of signal to noise for each voltage is show below:&lt;br /&gt;
&lt;br /&gt;
[[File:2.6-9_sig_noi_ratio.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
 You need to add error bars and make measurements at additional voltages &lt;br /&gt;
 ( measure for every 5 volts if error bars can tell the difference between each voltage)&lt;br /&gt;
&lt;br /&gt;
It is noticed that increasing the voltage decreased the signal to noise ratio unless it is within the error bars, also increasing the voltage of the GEM from 2.87 to 2.97 kV does not affect the noise signal ratio, but it increases the charge detected which is expected as main characteristic for the GEM preamp. (results are same using both definitions of signal to noise ratio).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| V_GEM (kV) || open || closed || notes&lt;br /&gt;
|-&lt;br /&gt;
|2.87     || 8479,8481, 8408 || 8480,8482,8409&lt;br /&gt;
|-&lt;br /&gt;
| 2.97  || 8484, 8486,8415 || 8483,8485,8416&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=12/30/14 Determining the noise level using pulse shape and peak sensing discrimination simultaneously =&lt;br /&gt;
&lt;br /&gt;
Using an AND-gate for a peak sensing discriminator and a leading edge one is used to determine the relationship between the discrimination level and the the signal rate.&lt;br /&gt;
&lt;br /&gt;
[[Psensing spectra with an AND-gate output as a gate for the module]]&lt;br /&gt;
&lt;br /&gt;
;Using LED only&lt;br /&gt;
&lt;br /&gt;
The LED disc. is used instead of the PS disc. to measure the Psensing charge spec., the following figure shows the result.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:LED_o_c_3_3.6kV.png |300px]]&lt;br /&gt;
&lt;br /&gt;
the signal is amplified so it is higher than the noise level, but still the LED disc. is unable to distinguish between open shutter and closed one.&lt;br /&gt;
&lt;br /&gt;
the noise level is measured and it is 78 mV. (run 8445)&lt;br /&gt;
&lt;br /&gt;
 The counts near channel 100 suggest that the leading edge discriminator is not rejecting noise that we called a pedestal event.&lt;br /&gt;
&lt;br /&gt;
=12/27/14 Peak shift with changing the GEM preamp. Voltage=&lt;br /&gt;
&lt;br /&gt;
==GEM3k peak sensing charge spectra==&lt;br /&gt;
&lt;br /&gt;
[[GEM3k peak sensing charge spectra]]&lt;br /&gt;
&lt;br /&gt;
;GEM 2.87kV and cath. 3.47kV&lt;br /&gt;
&lt;br /&gt;
[[File:CATH3.47_GEM2.87_8409c_8408.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
;GEM 2.67 and cath. 3.27kV&lt;br /&gt;
&lt;br /&gt;
[[File:CATH3.27_GEM2.67_8410c_8411.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;GEM 2.97 and cath. 3.57kV&lt;br /&gt;
&lt;br /&gt;
[[File:CATH3.57_GEM2.97_8416c_8415.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
=12/24/14 Peak shift with changing the GEM preamp. Voltage=&lt;br /&gt;
&lt;br /&gt;
The following figure shows the peak shift in the Peak sensing charge spectrum as Drfit voltage is 700 V and  the GEM voltage is changed as shown in the figure:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:peak_shift_G2.77_2.9kV_1.png | 300px]]&lt;br /&gt;
[[File:peak_shift_G2.77_2.9kV_2.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
The figure above shows the peak shift as the GEM preamp. voltage is 2.77kV and 2.9kV. the higher voltage for the GEM preamp., the higher charge collected from the detector. Also the noise peak rate at channel is less at a higher GEM voltage.&lt;br /&gt;
&lt;br /&gt;
=12/24/14 GEM_V = 2.82 kV=&lt;br /&gt;
&lt;br /&gt;
[[cathode drift potential and count rate runs for 2.82kV GEM]]&lt;br /&gt;
&lt;br /&gt;
=12/18/14 Comparing increasing the GEM voltage 30 V to 2.9 KV=&lt;br /&gt;
&lt;br /&gt;
;GEM_V= 2.87 kV&lt;br /&gt;
[[File:all_open_V_rate_GEM2.87kV.png | 400px]]&lt;br /&gt;
[[File:all_closed_V_rate_GEM2.87kV.png | 400px]]&lt;br /&gt;
[[File:all_sub_V_rate_GEM2.87kV.png | 400px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:all_fit_rate_sub_2.87kV.png | 400px]]&lt;br /&gt;
[[File:all_fit_rate_open_2.87kV.png | 400px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;GEM_V= 2.9 kV&lt;br /&gt;
&lt;br /&gt;
The results shows the integral under the charge spectra:&lt;br /&gt;
&lt;br /&gt;
[[File:all_open_V_rate_GEM2.9kV.png | 400px]]&lt;br /&gt;
[[File:all_closed_V_rate_GEM2.9kV.png | 400px]]&lt;br /&gt;
[[File:all_sub_V_rate_GEM2.9kV.png | 400px]]&lt;br /&gt;
&lt;br /&gt;
The maximum rate for the first peak in case of open shutter and in case of the subtraction is shown below: &lt;br /&gt;
&lt;br /&gt;
[[File:all_fit_rate_sub_2.9kV.png | 400px]]&lt;br /&gt;
[[File:all_fit_rate_open_2.9kV.png | 400px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Notes&lt;br /&gt;
&lt;br /&gt;
Increasing the the GEM voltage &lt;br /&gt;
&lt;br /&gt;
#Increased the charge as the shutter is open as the drift voltage is in between 600-800V &lt;br /&gt;
#Increased the rate of the first peak rate, the rate at 800V and 900 V is not the same for all runs, the latest runs have higher rate, and the error bars are bigger for 800 and 900V.&lt;br /&gt;
#There is not any difference in maximum rate of the first peak for open shutter and the subtraction, so the shutter is completely stopping the charge flow to the anode as it is closed, even after the GEM's voltage increment.&lt;br /&gt;
# I will upload more graphs that have the average for each figure for the two values of the GEM voltages.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; 2.87 kV and 2.9 kV&lt;br /&gt;
&lt;br /&gt;
[[File:averages_2.87_2.9_charge_int.png| 400px]]&lt;br /&gt;
&lt;br /&gt;
The figure above shows that increasing the GEM voltage with 30 V does not change the amount of charge except for the drift voltage in the range of 500 to 700 V (increase) and 900 to 1kV (decrease). The first peak rate in increases when the GEM voltage increases 30 V as the drfit voltage in the range of 300-900 V as shown below:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:averages_2.87_2.9_firstpeak.png| 400px]]&lt;br /&gt;
&lt;br /&gt;
=12/15/14=&lt;br /&gt;
&lt;br /&gt;
Data analysis,&lt;br /&gt;
&lt;br /&gt;
[[File:12_2_3_4_count_rate_cathV.xls]]&lt;br /&gt;
&lt;br /&gt;
=12/11/14=&lt;br /&gt;
&lt;br /&gt;
 you forgot to put possible reason for fluctuation in legend.  Listing the possible reasons below is not informative&lt;br /&gt;
&lt;br /&gt;
Figure 1.) Open-Closed data , from 10/25/14 -&amp;gt; 12/9/14, color code different days,  legend indicates date and possible reason for fluctuations.&lt;br /&gt;
 &lt;br /&gt;
[[File:all_sub_V_rate.png |400px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Figure 2.) Open data , from 10/25/14 -&amp;gt; 12/9/14, color code different days,  legend indicates date and possible reason for fluctuations.&lt;br /&gt;
&lt;br /&gt;
[[File:all_open_V_rate.png |400px]]&lt;br /&gt;
&lt;br /&gt;
Figure 3.) Closed data , from 10/25/14 -&amp;gt; 12/9/14, color code different days,  legend indicates date and possible reason for fluctuations.&lt;br /&gt;
&lt;br /&gt;
[[File:all_Closed_V_rate.png |400px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Fluctuations&lt;br /&gt;
&lt;br /&gt;
#Changing the bottle twice.&lt;br /&gt;
# Weather temperature.&lt;br /&gt;
# Ar/CO2 gas' temperature was lower than the lab's temperature for the last bottle, a change is observed before and after the 11/20/14. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Figure 4.) Open-Closed data , from 10/9-present, color code different days,  legend indicates date and possible reason for fluctuations.&lt;br /&gt;
&lt;br /&gt;
Figure 5.) Open data , from 10/9-present, color code different days,  legend indicates date and possible reason for fluctuations.&lt;br /&gt;
&lt;br /&gt;
Figure 6.) Closed data , from 10/9-present, color code different days,  legend indicates date and possible reason for fluctuations.&lt;br /&gt;
&lt;br /&gt;
; The effect of the drift field &lt;br /&gt;
&lt;br /&gt;
[[File: Laura De Nardo, Marchiori Elena, PhD thesis,Università degli studi di Padova, 2013/2014]]&lt;br /&gt;
&lt;br /&gt;
There is an effect for the drift potential on the count rate as its value is less than 0.4 kV, one of the reasons that the drift force line ends on the surface of the GEM electrode, on the other hand, when the drift more than 0.4 kV, the drift force lines converge inside the hole.&lt;br /&gt;
&lt;br /&gt;
Another reason is in case of the drift potential is more than 0.4 kV, the probability of electron-ion recombination before the GEM electrode is less compared to the case when the drift potential is less than 0.4 kV. &lt;br /&gt;
&lt;br /&gt;
If the electric field is higher than 0.8 kV, the electric filed lines end on the surface, and the ones in the holes do not converge as much as in the case of of V_drift =&amp;lt; 0.8 kV, which cause an electron defacusing effect.&lt;br /&gt;
&lt;br /&gt;
[[File:bachmann_GEM_charge_transcfer_properties_driftE.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:DriftV_amp.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
=12/10/14=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Three figures&lt;br /&gt;
&lt;br /&gt;
Figure 1.) Open-Closed data , from 10/25/14 -&amp;gt; 12/9/14, color code different days,  legend indicates date and possible reason for fluctuations.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Figure 2.) Open data , from 10/25/14 -&amp;gt; 12/9/14, color code different days,  legend indicates date and possible reason for fluctuations.&lt;br /&gt;
&lt;br /&gt;
Figure 3.) Closed data , from 10/25/14 -&amp;gt; 12/9/14, color code different days,  legend indicates date and possible reason for fluctuations.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Figure 4.) Open-Closed data , from 10/9-present, color code different days,  legend indicates date and possible reason for fluctuations.&lt;br /&gt;
&lt;br /&gt;
Figure 5.) Open data , from 10/9-present, color code different days,  legend indicates date and possible reason for fluctuations.&lt;br /&gt;
&lt;br /&gt;
Figure 6.) Closed data , from 10/9-present, color code different days,  legend indicates date and possible reason for fluctuations.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:cath_3.47kV_2.87kV_rate_date.png || 300px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Figure 7.) Overlay average of 10/25/14-&amp;gt; 12/9/10 measurements and average of 10/9-present, legend indicated GEM voltage,&lt;br /&gt;
&lt;br /&gt;
=12/09/14=&lt;br /&gt;
&lt;br /&gt;
[[File:count_rate_GEM_2.9kV_12_08_09_ave.png |300px]] &lt;br /&gt;
[[File:count_rate_GEM_2.9kV_12_09.png |300px]] &lt;br /&gt;
[[File:count_rate_GEM_2.9kV_12_08.png |300px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Reference for number pf counts vs the cathode voltage&lt;br /&gt;
&lt;br /&gt;
=12/08/14  2.9kV GEM =&lt;br /&gt;
&lt;br /&gt;
[[cathode drift potential and count rate runs for 2.9kV GEM]]&lt;br /&gt;
&lt;br /&gt;
=12/08/14=&lt;br /&gt;
The figure shows the drift voltage vs the count rate in another weekend.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:  12_07_cath_rate_count.png| 300px]]&lt;br /&gt;
&lt;br /&gt;
The graph is different from the graph taken by the previous weekend 11/29/14 as the drift potential is less than 350 V. as shown below&lt;br /&gt;
&lt;br /&gt;
11/29[[File:  11_29_cath_rate_count.png| 300px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Investigate ionized electron transmission by looking at previous published studies of Cathode voltage differences.&lt;br /&gt;
&lt;br /&gt;
=12/05/14=&lt;br /&gt;
&lt;br /&gt;
;Beta Transmission ratio percentage in FR4&lt;br /&gt;
&lt;br /&gt;
The figure below shows the number of beta transmitted through 1 mm FR4, the collected data considers only the incident beta only without counting for primary electrons as result of the ionization through the shutter and without electron ionization in the gas in the drift volume.&lt;br /&gt;
&lt;br /&gt;
[[File:  Beta_FR4_trans_EkeV_percent.png | 300px]][[File:TABeta_FR4_trans_EkeV_percent.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Cathode vs Count Rate&lt;br /&gt;
&lt;br /&gt;
11/29[[File:  11_29_cath_rate_count.png| 300px]]&lt;br /&gt;
&lt;br /&gt;
The figure shows the count rate as the shutter is open (green), closed (red), and their subtraction (blue) as the drift voltage changes. The measurements were taken in the weekend.&lt;br /&gt;
&lt;br /&gt;
12/02[[File:  12_02_cath_rate_count.png| 300px]]&lt;br /&gt;
12/03[[File:  12_03_cath_rate_count.png| 300px]]&lt;br /&gt;
12/04[[File:  12_04_cath_rate_count.png| 300px]]&lt;br /&gt;
&lt;br /&gt;
The figures above show the count rate in three different working days, the color refernce is as the figure above.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:  12_ave_cath_rate_count.png| 300px]]  [[File:12_2_3_4_count_rate_cathV.xls ]]  &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The average of previous of the data for the three figures above is calculated with the error bars.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Notes:&lt;br /&gt;
&lt;br /&gt;
# As mentioned below, as the drift potential is between 400-900V, the same count rate is measured in average for the the three cases.&lt;br /&gt;
#The count rate increase between 193V and 200V was not observed.&lt;br /&gt;
#As the voltage is 900V, in all days, a high noise is observed for shutter open. It confirms what we discussed before; it indicates a need for more amplification and a higher discrimination level if we are interested in determining the full charge spectrum from  U-233.&lt;br /&gt;
#Another set of measurements will be taken this weekend to reproduce the graph for 11/29.&lt;br /&gt;
&lt;br /&gt;
=12/01/14=&lt;br /&gt;
&lt;br /&gt;
The figure shows the drift voltage effect on the number of counts for shutter open (green), closed (red), and their subtraction (blue)&lt;br /&gt;
&lt;br /&gt;
[[File:  11_29_cath_rate_count.png| 300px]]&lt;br /&gt;
&lt;br /&gt;
I noticed:&lt;br /&gt;
&lt;br /&gt;
# There is not any effect for increasing the cathode voltage when the drift voltage is 400V or higher.&lt;br /&gt;
# The count rate is doubled between as the drift voltage changes from 193V to 200V.&lt;br /&gt;
# Compared to the previous graph (measurements before 11/20/14) a shift in the voltage for the area that number of count rate dramatically increased, it changed  from around 600V to 200V. Also the count rate decreased with about 10Hz (only for the subtraction graph in blue) after changing the old bottle.&lt;br /&gt;
# The data are measured in the weekend, and it would be measured again through the normal working days to compare the results.&lt;br /&gt;
&lt;br /&gt;
=11/29/14 Electron range in FR4=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: e_EkeV_FR4_range_cm.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
The calculations considers the excitation energy for FR4 equals to 107.1 eV.[http://physics.nist.gov/PhysRefData/Star/Text/ESTAR.html], and composite is from the site [http://personalpages.to.infn.it/~tosello/EngMeet/ITSmat/SDD/SDD_G10FR4.html]&lt;br /&gt;
&lt;br /&gt;
=11/25=&lt;br /&gt;
&lt;br /&gt;
[[File:Cath_volt_count_before_11_19_all.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
=11/03-19 Ionization calculations=&lt;br /&gt;
&lt;br /&gt;
[[File:total_ionization_3particles.xls]]&lt;br /&gt;
&lt;br /&gt;
=11/20/14=&lt;br /&gt;
&lt;br /&gt;
A difference in the number is noticed after changing to the new bottle!!!!!&lt;br /&gt;
&lt;br /&gt;
[[File:Cath_volt_count.png | 300px]]&lt;br /&gt;
[[File:Cath_volt_count_after_11_19.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
=10/27/14=&lt;br /&gt;
&lt;br /&gt;
Plot&amp;lt;math&amp;gt; \Delta&amp;lt;/math&amp;gt; V -vs- R&lt;br /&gt;
&lt;br /&gt;
 The &amp;lt;math&amp;gt;\Delta&amp;lt;/math&amp;gt; V -vs-  R  graph seems to be jumping around a lot.  &lt;br /&gt;
 This may mean we need more measurements in order to determine if there is a smooth dependence or not&lt;br /&gt;
&lt;br /&gt;
[[File:Cath_volt_count.png | 300px]]&lt;br /&gt;
[[File:Cath_volt_rate.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Ar ionization cross section&lt;br /&gt;
&lt;br /&gt;
The energy is in the unit of MeV/amu which is relative to the atomic mass unit of hte target. In our case we are interested in Ar which has an  amu = 40.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: Ar_e_ionization_xsection_10MeV.png  | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=10/24/14=&lt;br /&gt;
&lt;br /&gt;
Table of Histograms with NO SOURCE, shutter open and closed, and changing V cathode&lt;br /&gt;
&lt;br /&gt;
(750 Volts)&lt;br /&gt;
&lt;br /&gt;
Plot the rate of all three particles from source onto one plot&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:3particles_energy.png |200px]]  [[File:U-33_SourceParticlePercentage.xmgrace.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electron energy threshold to penetrate  1mm thick FR4, and the energy for full penetration.&lt;br /&gt;
&lt;br /&gt;
Plot transmission by taking ratio of (Number particle through shutter)/(Number of particles hitting shutter)&amp;lt;math&amp;gt; \frac{N_{trans}}{N_{inc}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Plot Energy loss ( 100 *&amp;lt;math&amp;gt; \frac{E_i-E_f}{E_i}&amp;lt;/math&amp;gt;)&lt;br /&gt;
&lt;br /&gt;
=10/23/14=&lt;br /&gt;
&lt;br /&gt;
Table of Histograms with NO SOURCE, shutter open and closed, and changing V cathode&lt;br /&gt;
&lt;br /&gt;
=10/22/14=&lt;br /&gt;
&lt;br /&gt;
[[ Long run peak sensing histograms ]] &lt;br /&gt;
&lt;br /&gt;
[[ 20min run peak sensing histograms ]]&lt;br /&gt;
&lt;br /&gt;
= 20 min. GEM-2.87 kV CATH-3.435 kV 10/17/14=&lt;br /&gt;
&lt;br /&gt;
 you need to label the axis and color code the statistics box so I know which distribution corresponds to which configuration.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Date ||Shutter || source || run number || Scaler counts (Hz)  || pedestal || Integral in ADC full spectrum (Hz)  || Integral in ADC spectrum beyond pedestal (Hz)|| notes&lt;br /&gt;
|-&lt;br /&gt;
|10/16|| Open ||off || 7847|| 150+_7 || 1429/60 ||  7915/60 || 5810/60&lt;br /&gt;
|-&lt;br /&gt;
| 10/16||Closed || off || 7846||72+_3  || 1070/60 || 4029/60 || 2817/60&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
| 10/16 || Open || off || 7848|| 137+_16 || 19 ||  129 || 111 || [[File:4runs_7848_62_63_64.png | 200px]]&lt;br /&gt;
|-&lt;br /&gt;
| 10/16|| Closed ||  off || 7862|| 53+_1 || 7 ||  47|| 41&lt;br /&gt;
|-&lt;br /&gt;
|10 /16 || Open || On || 7863|| 147+_12|| 30 ||  129 || 101&lt;br /&gt;
|-&lt;br /&gt;
| 10/16 || Closed || On ||  7864|| 67+_4 || 15 || 59 || 45&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 10/17 || Open || off || 7865|| 132+_14 || 28 || 121  || 97 ||  [[File:4runs_7865_66_68_67.png| 200px]]&lt;br /&gt;
|-&lt;br /&gt;
| 10/17|| Closed ||  off || 7866|| 95+_7 || 11 || 59 || 49&lt;br /&gt;
|-&lt;br /&gt;
|10 /17 || Open || On || 7868|| 150+_6|| 32 || 128  || 100&lt;br /&gt;
|-&lt;br /&gt;
| 10/17 || Closed || On ||  7867||74+_4 || 13 || 63 || 52&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 10/18 || Open || off || 7872|| 136+_10 || 9 || 124  || 115 || [[File:4runs_7872_71_69_70.png| 200px]]&lt;br /&gt;
|-&lt;br /&gt;
| 10/18|| Closed ||  off || 7871|| 51+_3 || 4 || 48 || 44&lt;br /&gt;
|-&lt;br /&gt;
|10 /18 || Open || On || 7869|| 140+_10|| 10 || 123  || 115&lt;br /&gt;
|-&lt;br /&gt;
| 10/18 || Closed || On ||  7870||53+_2 || 4 || 49 || 44&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 10/19 || Open || off || 7873|| 124+_14 || 10 || 114  || 104 || [[File:4runs_7873_74_76_75.png| 200px]]&lt;br /&gt;
|-&lt;br /&gt;
| 10/19|| Closed ||  off || 7874|| 59+_4 || 5 || 54 || 49&lt;br /&gt;
|-&lt;br /&gt;
|10 /19 || Open || On || 7876|| 141+_8|| 10 || 117  || 108&lt;br /&gt;
|-&lt;br /&gt;
| 10/19 || Closed || On ||  7875||60+_4 || 6|| 55 || 50&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 10/20 || Open || off || 7879|| 129+_16 || 8 || 116  || 108 ||[[File:4runs_7879_80_82_81.png | 200px]]&lt;br /&gt;
|-&lt;br /&gt;
| 10/20|| Closed ||  off || 7880|| 49+_2 || 2 || 45 || 42&lt;br /&gt;
|-&lt;br /&gt;
|10 /20 || Open || On || 7882|| 142+_3|| 8 || 108  || 99&lt;br /&gt;
|-&lt;br /&gt;
| 10/20 || Closed || On ||  7881||53+_2 || 5|| 49 || 44&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=10/16/14=&lt;br /&gt;
&lt;br /&gt;
 you need to label these histograms with more detail that will identify the run number and the run conditions.  &lt;br /&gt;
 Name each histogram according to the run number then in a figure caption identify the run conditions.&lt;br /&gt;
&lt;br /&gt;
 you need to show more than just 4 runs, try to take 10, why is the pedestal peak different in the four that you show.&lt;br /&gt;
&lt;br /&gt;
 You need to have units of Hz for the count rate on the y-axis.&lt;br /&gt;
&lt;br /&gt;
  I should not be asking you for the above things at this stage of your career, you should be doing hem automatically&lt;br /&gt;
&lt;br /&gt;
  I am not giving any formal results yet since the voltage of the GEM may increase.&lt;br /&gt;
&lt;br /&gt;
 The point is to able to understand what is plotted and have a reference to fall back on&lt;br /&gt;
&lt;br /&gt;
  Formal results will be even more detailed &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Last update for the today's measurements:&lt;br /&gt;
&lt;br /&gt;
# Reproduciblity is achieved when for the peak sensing spectra for shutter open and shutter close without source.&lt;br /&gt;
# Increasing the GEm amplification is needed for the case of the shutter open with the source on.&lt;br /&gt;
&lt;br /&gt;
[[File:10_16_14_4runs.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
Analyze all runs with same conditions of HV, Gas, …  to determine the integral number of counts in  the ADC(PADC) histogram that are above the pedestal.&lt;br /&gt;
&lt;br /&gt;
=10/14-15/14=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Shutter || run numbers || average number of counts above the pedestal&lt;br /&gt;
|-&lt;br /&gt;
|Open ||  7797, 7802, 7808, 7816 || [[File:sh.open_1stpeak_int.png |200px]] [[File:sh.open_2ndpeak_int.png |200px]]&lt;br /&gt;
|-&lt;br /&gt;
|Closed || 7798, 7803, 7809, 7817 || [[File:sh.closed_1stpeak_int.png |200px]] [[File:sh.closed_2ndpeak_int.png |200px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Fix the percentage plot for the number of betas emitted by the source.&lt;br /&gt;
&lt;br /&gt;
The repcentages do not add to 100% according to two different references.[http://t2.lanl.gov/nis/data/endf/decayVII.1.html][http://www.nndc.bnl.gov/nudat2/index.jsp]&lt;br /&gt;
they add to about 20%, the first referece bentioned that the average energy for the emitted particles from U-233 are&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Ebeta (eV)   : 5.043230e+3 (5.363190e+2)&lt;br /&gt;
&lt;br /&gt;
Egamma (eV)  : 1.110210e+3 (1.076780e+2)&lt;br /&gt;
&lt;br /&gt;
Ealpha (eV)  : 4.888350e+6 (2.896760e+4)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Fix the alpha log plot for cross-section, change units on the beta plot for cross section so they are in barns.&lt;br /&gt;
&lt;br /&gt;
Add plot for expected voltage on oscilloscope.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Alpha || [[File: alpha_energy_percentages.png  | 300 px]] ||[[File: Ar_alpha_ionization_xsection.png  | 300 px]] || [[File: alpha_primaries.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
| Beta||  [[File: beta_energy_percentages.png  | 300 px]]  || [[File: Ar_e_ionization_xsection.png  | 300 px]][http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1967ApJS...14..207L&amp;amp;db_key=AST&amp;amp;page_ind=0&amp;amp;plate_select=NO&amp;amp;data_type=GIF&amp;amp;type=SCREEN_GIF&amp;amp;classic=YES] [[File:Ar_e_ionization_ref_p1.gif |10 px]]  &lt;br /&gt;
 || &lt;br /&gt;
|-&lt;br /&gt;
| Gamma || [[File: gamma_energy_percentages.png  | 300 px]] || [[File: Ar_gamma_ionization_xsection.png  | 300 px]] || [[File: gamma_primaries.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=10/13/14=&lt;br /&gt;
&lt;br /&gt;
 stripchart&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Relationship between barns and g/cm^2&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; macroscopic \,\, xsection (cm^2/g) = \frac{6.022 \times 10^{23}}{atomic mass} * xsections \,\, (cm^2)) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 paragraph describing percentage plots for alpha, beta, and gamma with references.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|long run || time || shutter || source || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7832 || 6h || open || off || 8dB&lt;br /&gt;
|-&lt;br /&gt;
|7834 || 35min || closed || off || 8dB&lt;br /&gt;
|-&lt;br /&gt;
|7836 || 5.5h || open || on || 11 dB&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=10/10/14=&lt;br /&gt;
&lt;br /&gt;
=10/02/14=&lt;br /&gt;
QDC's and Peak sensing's spectra distinguish between shutter open and shutter close as the source is on, I noticed it from yesterday's and today's measurements.&lt;br /&gt;
&lt;br /&gt;
Also the spectra shows a difference in the number of count and the number of channels as the source on or off as the shutter is open. more measurements is needed to calculate the STDEV.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The oscilloscope picture is shows the gate and signal details,&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| date || time run ended || Source || run number|| notes&lt;br /&gt;
|-&lt;br /&gt;
|  10/02/14||  10:45  || On || 7792  || each run time is 20 min.&lt;br /&gt;
|-&lt;br /&gt;
| 10/02/14 || 11:07 || off || 7793      || 22', taking the source off directly then measuring the charge does not show any difference in channel number but shows difference in counts.&lt;br /&gt;
|-&lt;br /&gt;
| 10/02/14 || 16:30 || off || 7795     || 20', after 5 1/2 h  the detector started to show a little difference again between shutter open source is on and when the source is off.&lt;br /&gt;
|-&lt;br /&gt;
| 10/03/14 || 8:00 || off || 7795     || 20'&lt;br /&gt;
|-&lt;br /&gt;
| 10/03/14 || 11:21|| off || 7795     || 20'  equilibrium without source.&lt;br /&gt;
|-&lt;br /&gt;
| 10/06/14 || 09:05|| off || 7802     || 20'  equilibrium without source.&lt;br /&gt;
|-&lt;br /&gt;
| 10/07/14 || 7:00|| off || 7806     || lower charge is detected &lt;br /&gt;
|-&lt;br /&gt;
| 10/07/14 || 11:19|| off || 7807     || higher charge is detected (TSO's stuff were checking on the source)&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM_HV= 2870 Volts, Drift HV =  3470 Volts&lt;br /&gt;
&lt;br /&gt;
[[File:GEMoutput_10022014_A.png | 200 px]]&lt;br /&gt;
[[File:GEMoutput_10022014_B.png | 200 px]][[File:GEMoutput_10022014_C.png | 200 px]]&lt;br /&gt;
&lt;br /&gt;
=09/30/14=&lt;br /&gt;
&lt;br /&gt;
Plot of shutter open/closed (NO SOURCE) counter rate -vs- date&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha's Primaries&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_energy_percentages.png  | 300 px]]&lt;br /&gt;
[[File: Ar_alpha_ionization_xsection.png  | 300 px]]&lt;br /&gt;
[[File: alpha_primaries.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
[[File:alpha_primaries.xls]]&lt;br /&gt;
&lt;br /&gt;
Plot of Number of electrons collected -vs- Energy of (alpha, beta, and gamma) from U-233&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: beta_energy_percentages.png  | 300 px]]&lt;br /&gt;
[[File: Ar_e_ionization_xsection.png  | 300 px]]&lt;br /&gt;
[[File: Ar_e_ionization_xsection_10MeV.png  | 300 px]] [K Paludan et al 1997 J. Phys. B: At. Mol. Opt. Phys. 30 L581 doi:10.1088/0953-4075/30/17/005&lt;br /&gt;
]&lt;br /&gt;
&lt;br /&gt;
[http://www.example.com link title]&lt;br /&gt;
[[File:e_stoppingpower_MeV_MeVcmg-2.png | 300 px]]&lt;br /&gt;
[[File: Ar_e_range_MeV_gcm-2.png  | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Gamma&lt;br /&gt;
&lt;br /&gt;
[[File: gamma_energy_percentages.png  | 300 px]]&lt;br /&gt;
[[File: Ar_gamma_ionization_xsection.png  | 300 px]]&lt;br /&gt;
[[File: gamma_primaries.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=09/29/14=&lt;br /&gt;
&lt;br /&gt;
; Shutter open/close data plot for 2.87 3.48 kV GEM /Cathode&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://www.nndc.bnl.gov/chart/decaysearchdirect.jsp?nuc=233U&amp;amp;unc=nds] The reference gives percentages of the emitted alpha particles as U-233 -&amp;gt; Th229 [[File:alpha percentages.txt]]&lt;br /&gt;
&lt;br /&gt;
[[File:alpha_E_percent.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Roy's detector infomation and measurements&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
[[File: Alpha_Secondaries.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;09/20/14&lt;br /&gt;
&lt;br /&gt;
Rate of ( alpha, photon, beta) -vs- energy for U-233&lt;br /&gt;
&lt;br /&gt;
Primary electron ionization -vs- (alpha,photon, beta) energy&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Secondaries&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Photo-Absorption Secondaries&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: Photo-Absorption Secondaries.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
The reason that the graph started from 30 keV  is the lowest gamma energy emitted by U-233 or Cf-252 is higher than that energy.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electron Ionization&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Using NIST data base [http://physics.nist.gov/cgi-bin/Ionization/table.pl?ionization=CO2]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
we got the following data file for CO2 [[File:CO2_e_ionization_xsection.txt]], For Ar, the ref. [http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1967ApJS...14..207L&amp;amp;db_key=AST&amp;amp;page_ind=0&amp;amp;plate_select=NO&amp;amp;data_type=GIF&amp;amp;type=SCREEN_GIF&amp;amp;classic=YES] that measured the ionization xsection. [[File:Ar_e_ionization_ref_p1.gif |10 px]]  [[File:Ar_e_ionization_ref_p1.gif |10 px]]&lt;br /&gt;
&lt;br /&gt;
[[File:Ar_e_ionization_xsection.gif | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=09/20/14=&lt;br /&gt;
&lt;br /&gt;
The figure below shows the change in the signal as the GEM capacitor charges, at a specific fixed voltage it reaches saturation (equilibrium),&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_signal_time_equilibS.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
If the capacitor does not reach equilibrium, the signal of the detector is expected to change with time.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
  What may forbid the GEM capacitor to reach the equilibrium?&lt;br /&gt;
&lt;br /&gt;
# The circuit board voltage fluctuations.&lt;br /&gt;
#The following reference describes almost the same conditions as those of our detector when their detector is in operation to detect simultaneously photons with alpha particles.&lt;br /&gt;
&lt;br /&gt;
Nuclear Instruments and Methods in Physics Research A 471 (2001) 151–155 &lt;br /&gt;
&lt;br /&gt;
[[File:gas electron multiplier for portal imaging_wallmark.pdf]]&lt;br /&gt;
&lt;br /&gt;
The author commented in the conclusion &amp;quot;The studies show that GEMs can operate at extremely high rates (&amp;gt;10^6 Hz/mm^2) with no sign&lt;br /&gt;
of degradation and '''stability loss''' due to radiation damage. However, &lt;br /&gt;
'''it was discovered that the maximum achievable gain for all planar gaseous detectors drops with the beam intensity''' &amp;quot;&lt;br /&gt;
&lt;br /&gt;
&amp;quot;In real clinical operation the detector can operate safely with a gain of 10^2 in the GEM closest to the collector&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
  Our detector has a rate of 100-170 Hz (without and with the source), considering  the detector age, will this rate cause an instability?&lt;br /&gt;
#High detector rate.&lt;br /&gt;
[[File:Fonte_GD_limitations.pdf]]&lt;br /&gt;
&lt;br /&gt;
The gain will decrease when the count rate increases, if GEMs' voltage is at the point where gain is stable with the high rate, the detector output will be reproducible. As mentioned above, a gain of 10^2 made it enough for imaging with a well-quenched gas, I doubt we need to increase the gain more than that.&lt;br /&gt;
&lt;br /&gt;
=9/18/14=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Determine best Cathode HV that produces the largest separation of the source ON/OFF signal.&lt;br /&gt;
&lt;br /&gt;
The detector results are not reproducible, as the voltage is at 3.4  kV, the QDC spectrum  is different as the source on; so QDC can not distinguish if the source is on or when it is off the detector.&lt;br /&gt;
&lt;br /&gt;
 Something is wrong!!!!&lt;br /&gt;
&lt;br /&gt;
We never have a reproducibility problem before using the QDC until I start using V1495, Can we borrow the older module just to test the reproducibility is still a problem. &lt;br /&gt;
&lt;br /&gt;
 It is very unlikely that it is the v1495.  The V1495 only tells the DAQ to read out a module.  &lt;br /&gt;
 You can test the DAQ by injecting a pulse with a known charge and look for it in the QDC spectrum.&lt;br /&gt;
&lt;br /&gt;
 It is VERY important to have scope pictures showing the difference between source ON/OFF.&lt;br /&gt;
 Then you use scalers to check that your trigger pulse is able to see a difference between source ON/OFF&lt;br /&gt;
 Then you do the DAQ measurements.  &lt;br /&gt;
&lt;br /&gt;
 If you don't follow the above proceedure then you will be building a pyramid on quicksand.&lt;br /&gt;
&lt;br /&gt;
The same case when the cathode voltage increased to 3.6 kV.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Then perform a set of measurements (shutter open/closed and source ON/OFF) to establish reproduceability.  Make sure you record the scaler count rates.&lt;br /&gt;
&lt;br /&gt;
=9/17/14=&lt;br /&gt;
&lt;br /&gt;
Measure the charge for several values of the Cathode HV keeping the GEM preamplifier voltage and gas flow rate constant.&lt;br /&gt;
&lt;br /&gt;
;CATH 3.2 KV&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7728_7729.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;CATH 3.1 KV&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7736_7737.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
All the runs have  the same duration 20 min.&lt;br /&gt;
&lt;br /&gt;
;CATH 3.4 KV&lt;br /&gt;
&lt;br /&gt;
Try to take scope picture to show difference between source on and off signal that are being measured by the QDC.&lt;br /&gt;
&lt;br /&gt;
=9/16/14=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Condition of above results&lt;br /&gt;
&lt;br /&gt;
Shutter is Open &lt;br /&gt;
&lt;br /&gt;
Red is Cf-252 source ON Run 7724&lt;br /&gt;
&lt;br /&gt;
Green is Cf-252 source OFF run 7726&lt;br /&gt;
&lt;br /&gt;
HV_GEM= -2930 Volts&lt;br /&gt;
HV_Cathode=-3400 Volts&lt;br /&gt;
&lt;br /&gt;
Gas Flow rate = 0.1 ft^3/hr&lt;br /&gt;
&lt;br /&gt;
;Goal:&lt;br /&gt;
&lt;br /&gt;
:Can the Cf-252 source ON signal be changed?&lt;br /&gt;
&lt;br /&gt;
Change the Cathode voltage to try and turn off the signal when the source is on.&lt;br /&gt;
&lt;br /&gt;
;Result&lt;br /&gt;
&lt;br /&gt;
Yes, when the cathode voltage is decreased  to -3100V, QDC histogram does not show any difference in the collected charge as the shutter is open with the source on it, and when the shutter is open without the source. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The figure below shows the change in the QDC spectrum when the cathode voltage is -3.2 kV.&lt;br /&gt;
[[File: QDC_source_on_off_7728_7729.png | 300 px]]&lt;br /&gt;
&amp;lt;references/&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
[[Neutron_TGEM_Detector_Abdel]]&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101201</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101201"/>
		<updated>2015-06-17T21:10:04Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was before the neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101200</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101200"/>
		<updated>2015-06-17T21:00:48Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9037 || 06/17 14:59 || 06/17 14:09|| 10 || open || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
}&lt;br /&gt;
&lt;br /&gt;
The charge spectrum returned to were it was beforet he neutron exposure after 29 days for closed shutter.&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101199</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101199"/>
		<updated>2015-06-17T20:54:21Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
}&lt;br /&gt;
&lt;br /&gt;
the charge spectrum returned to were it was beforet he neutron exposure after 29 days.S&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101198</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101198"/>
		<updated>2015-06-17T20:51:47Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9035 || 06/15 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9036 || 06/17 14:48 || 06/17 14:58|| 10 || closed || off || 28 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101193</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101193"/>
		<updated>2015-06-16T03:08:52Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV (ISU power shutdown)&lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/15 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 21:06 || 06/13 21:16|| 10 || closed || off || 27 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101192</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101192"/>
		<updated>2015-06-16T03:01:16Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9034 || 06/15 20:55 || 06/13 21:05|| 10 || open || off || 45 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101191</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101191"/>
		<updated>2015-06-13T18:56:40Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || closed || off || 26 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101190</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101190"/>
		<updated>2015-06-13T18:49:39Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
|9032 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 87 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
|9033 || 06/13 12:35 || 06/13 12:45|| 10 || open || off || 50 ||  GEM2.8kV 3.5kV &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101126</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101126"/>
		<updated>2015-05-26T19:30:15Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2.9kV 3.6kV &lt;br /&gt;
|-&lt;br /&gt;
|9024 || 05/26 13:20 || 05/26 13:27|| 7 || closed || off || 26 ||  GEM2.8kV 3.5kV (beta effect decreased) &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101125</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101125"/>
		<updated>2015-05-26T19:20:09Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/26 13:17|| 11 || open || off || 87 ||  GEM2,9kV 3,6kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101124</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101124"/>
		<updated>2015-05-26T19:16:12Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
|-&lt;br /&gt;
|9023 || 05/26 13:06 || 05/ || || open || off || 87 ||  GEM2,9kV 3,6kV &lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101116</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101116"/>
		<updated>2015-05-25T19:15:46Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 15:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101109</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101109"/>
		<updated>2015-05-23T21:41:47Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 3:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || high beta effect&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || high beta effect&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101108</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101108"/>
		<updated>2015-05-23T19:58:12Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 3:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9010 || 05/21 23:23 ||  05/22 10:00 || || closed || off || 30 || &lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101099</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101099"/>
		<updated>2015-05-20T02:01:26Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 3:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on || 30 || &lt;br /&gt;
|-&lt;br /&gt;
|9008 || 05/18 21:46 ||  05/19 19:59 || || closed || off || 30 || &lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101082</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101082"/>
		<updated>2015-05-19T03:45:54Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 3:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||  05/18 19:20 || || closed || on ||  || &lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101081</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101081"/>
		<updated>2015-05-18T04:22:01Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Last runs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 3:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/17 22:18  || || open || on ||  48|| &lt;br /&gt;
|-&lt;br /&gt;
|9007 || 05/17 22:23 ||   || || closed || on ||  || &lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101080</id>
		<title>Neutron TGEM Detector Abdel</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Neutron_TGEM_Detector_Abdel&amp;diff=101080"/>
		<updated>2015-05-16T17:04:03Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* QDC TDC PS-ADC setup */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[HM_2014]]&lt;br /&gt;
&lt;br /&gt;
[[2012]]&lt;br /&gt;
&lt;br /&gt;
[[2011]]&lt;br /&gt;
&lt;br /&gt;
[[2010]]&lt;br /&gt;
&lt;br /&gt;
[[2009]]&lt;br /&gt;
&lt;br /&gt;
= Last runs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|9005 || 05/15 3:00 || 05/16 10:55 || || open || off || 50 || &lt;br /&gt;
|-&lt;br /&gt;
|9006 || 05/16 10:57 || 05/16  || || open || on ||  || &lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=QDC TDC PS-ADC setup=&lt;br /&gt;
&lt;br /&gt;
;Peak sensing gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_PS_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC gate&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_QDC_gate.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC start&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_pulser.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;TDC STOP&lt;br /&gt;
&lt;br /&gt;
[[File: TDC_GEM.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;QDC shows a difference&lt;br /&gt;
&lt;br /&gt;
[[File: QDC_source_on_off_7724_7726.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Measurements of the frequently used gas mixture 90/10 Ar/CO2 for the second peak =&lt;br /&gt;
&lt;br /&gt;
;Changes from the former set up&lt;br /&gt;
&lt;br /&gt;
# Using the eG&amp;amp;G timing filter amp. 474 instead of the spectroscopic amp. to amplify the input for the peak sensing ADC.&lt;br /&gt;
#Gate of a width of 4us has been delyed to track the second peak, as a result part of output spectrum is lost except for the delayed part within the gate width as shown in the figures below:&lt;br /&gt;
&lt;br /&gt;
;Lost&lt;br /&gt;
&lt;br /&gt;
[[File: PS_l1.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
;Detected&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: PS_d1.png | 300 px]][[File: PS_d2.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
|7435 || 08/24/14|| 19:30:48 || 19:55:32 || || open || on || 400 || a peak is noticed on channel 400&lt;br /&gt;
|-&lt;br /&gt;
|7436 || 08/24/14|| 19:59:05 || 20:40:11 || || open || off || 216 || the peak disappeared&lt;br /&gt;
|-&lt;br /&gt;
|7438 || 08/24/14|| 19:59:05 || 10:00:00 || || open || on || 0.0146 || triple coin., high noise, max. is ch 355&lt;br /&gt;
|-&lt;br /&gt;
|7444 || 08/25/14|| 21:17:25 ||  21:20:35|| || open || on || 230 || gate delay 700 ns, peak disappeared [[File: gate delay700ns.png | 300 px]]&lt;br /&gt;
|-&lt;br /&gt;
|7446 || 08/25/14|| 21:29:51|| 21:38:55 || || open || off ||  185 || does not count for P_B. peak disappeared &lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: shutteropen_sourceon_off.png | 300 px]]&lt;br /&gt;
&lt;br /&gt;
= unknown gas mixed bottle measurements=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
; Updates&lt;br /&gt;
&lt;br /&gt;
Changing the leading edge disc. to understand the Peak sensing and explain the cut int he peak sensing graph.&lt;br /&gt;
&lt;br /&gt;
Measuring the noise. by starting by low signal rate to distinguish the signal from the noise. &lt;br /&gt;
&lt;br /&gt;
; Channels and signals&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|device|| ch || input source&lt;br /&gt;
|-&lt;br /&gt;
| ADC || 5 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 7|| 15 ||  GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 5 || 11 ||  PMT Left&lt;br /&gt;
|-&lt;br /&gt;
| Peak sensing 8|| 17 ||  PMT right&lt;br /&gt;
|-&lt;br /&gt;
|PS translator ||&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 25 || PMT L&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|TDC|| 27 || GEM's trigout&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 29 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 31 (Stopper) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|CAEN N638&lt;br /&gt;
|-&lt;br /&gt;
|TDC || 17 || PMT L&lt;br /&gt;
|-&lt;br /&gt;
|TDC B2||  18|| GEM's trigout multi-hit&lt;br /&gt;
|-&lt;br /&gt;
|TDC B6||  22|| GEM's B_p&lt;br /&gt;
|-&lt;br /&gt;
| TDC || 21 || PMT R&lt;br /&gt;
|-&lt;br /&gt;
| TDC 6 || 30 (pulser) || triple coincidence (OR Mode)&lt;br /&gt;
|-&lt;br /&gt;
|TDC 7 ||  23|| delayed GEM's trigout&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Run Number||Date || start || end || Time (min) || Shutter || Source ||  Count rate (counts/min) || Notes&lt;br /&gt;
|-&lt;br /&gt;
| 7273|| 08/06/14 || 07:10:38 || 11:41:00 ||  12502 || open || off || 67 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7274|| 08/06/14 || 11:49:35 || 18:15:01 ||  23126 || closed || off || 39 || 0.1 flow rate&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7275|| 08/06/14 || 20:37:07 ||  09:10:10||   || closed || off || 40 || 0.2 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7276|| 08/06/14 || 09:15:00 ||  09:32:00||   || open || off || 80 || 0.2 flow rate amplification increases from 50 to 100&lt;br /&gt;
|-&lt;br /&gt;
| 7277|| 08/06/14 ||  09:33:08 || 11:40:42||  7654 || open || off ||  81 || 0.2 &lt;br /&gt;
|-&lt;br /&gt;
| 7295|| 08/08/14 ||  17:36:58 || 19:55:59|| 4741  || closed || off ||  60 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7296|| 08/08/14 ||  22:28:01 || 23:43:14||   || closed || off ||  58 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7297|| 08/08/14 ||  23:48:14|| 12:08:00  || 37186|| open || off ||  93 || 0.3 &lt;br /&gt;
|-&lt;br /&gt;
| 7298|| 08/09/14 ||  00:16:14||  06:08:03 ||21109 ||closed || off ||  56 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7299|| 08/10/14 ||  19:27:12||  20:09:04 || 2152||closed || on ||  107 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7300|| 08/10/14 ||  20:11:30||  20:46:29 ||2099 ||open || on ||  136 || 0.1 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7302|| 08/11/14 ||  06:53:14||  07:22:45 || 1771||closed || on ||  114 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7303|| 08/11/14 ||  07:26:58||  07:48:01 || 1263||open || on ||  167 || 0.2 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7305|| 08/11/14 ||  13:21:16||  13:55:05 || 2029||open || on ||  178 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7306|| 08/11/14 ||  14:41:00||  15:40:00 || 3540||closed || on ||  110 || 0.3 &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7307|| 08/14/14 ||  08:14:15||  08:20:39 || 384||closed || off ||  || 0.1 noise measurements (pulser only)&lt;br /&gt;
|-&lt;br /&gt;
| 7308|| 08/14/14 ||  08:22:43||  08:29:23 || ||open || off ||  1314 || 0.1 noise measurements (pulser only) same noise level as shutter closed (ch. 86) for Peak sensing ADC&lt;br /&gt;
|-&lt;br /&gt;
| 7309|| 08/14/14 || 08:35:09 || 09:45:37 || 4229  || open || off ||  || 0.1 flow rate was not exact, little less.&lt;br /&gt;
|-&lt;br /&gt;
| 7310|| 08/14/14 || 09:46:12 || 11:18:39 ||  5547 || open || off || 54 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7311|| 08/14/14 || 11:19:45 || 13:01:57 ||  6132 || open || off || 52 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7312|| 08/14/14 ||  13:10:50 || 14:28:07||  4637 || open || off || 72 || 0.1 flow rate was not exact, little less.&lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
| 7313|| 08/14/14 ||  14:30:24|| 15:38: 48||  4056  || open || off || 80 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7314|| 08/14/14 ||  15:41: 52||  16:46:55  || 3897|| open || on || 147 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7315|| 08/14/14 ||  16:49: 59||  19:14:30  ||8729|| open || on || 148 || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7316|| 08/14/14 ||  19:18:43 || 22:14:07  ||10596 || open || on ||147  || 0.1 flow rate as is used to be&lt;br /&gt;
|-&lt;br /&gt;
| 7317|| 08/14/14 ||  22:18:24 || 10:18:52  || 43220|| open || on ||  0.0095|| 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|-&lt;br /&gt;
| 7318|| 08/15/14 ||  10:24:00 || 12:42:23  || 8303|| open || on || 147  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7319|| 08/15/14 ||   12:46:14 || 15:46:09 || 10795|| open || on || 148  || 0.1 flow rate &lt;br /&gt;
|-&lt;br /&gt;
| 7323|| 08/15-16/14 ||   16:59:39 || 06:03:11 || 46970|| open || off || 0.0011  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
| 7329|| 08/16/14 ||   07:06:32 || 10:35:35 || 12543|| open || off || 83  || 0.1 flow rate, PMT's charge is measured for L and R&lt;br /&gt;
|-&lt;br /&gt;
| 7330|| 08/16/14 ||   10:41:58 || 12:48:33 || 7595 || open || on ||  146 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7331|| 08/16-17/14 ||    12:52:07 || 06:45:03 || 64384 || open || off || 0.0016  || 0.1 flow rate, triple coincidence, coda counted 111 but the data file is empty!&lt;br /&gt;
|-&lt;br /&gt;
| 7332|| 08/17/14 ||   06:52:26 || 07:04:45|| 739 || open || on || 1367   || 0.1 flow rate noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
| 7333|| 08/17/14 ||   07:05:50 || 08:53:54 ||  || open || on || 155  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| 7334|| 08/17/14 ||   08:57:02 || 13:13:38 ||  || open || off ||  82 || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
| 7337|| 08/17/14 ||   14:17:24 ||  14:30:29||  || open || on ||  1400 || 0.1 flow rate, GEM 2.92 kV , CATH 3.47kV(+50V),  noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
|7338|| 08/17/14 ||  14:31:37|| 16:17:45||  || open || on || 163  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7339|| 08/17/14 ||  16:20:25|| 16:35:45 || || open || off || 1368  || 0.1 flow rate, noise measurements with the wave generator&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7340|| 08/17/14 ||  16:37:01 || 20:33:04||  || open || off || 95  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7341|| 08/17-18/14 ||  20:40:16|| 06:18:43 || || open || off || 0.0015  || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7342|| 08/18/14 ||  06:25:44 || 06:37:43 || || open || on || 1403   || 0.1 flow rate, noise measurements&lt;br /&gt;
|-&lt;br /&gt;
|7345|| 08/18/14 ||  06:39:23 || 14:17:58 || || open || on ||0.0128   || 0.1 flow rate, triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7355|| 08/18/14 ||  16:03:29 ||  19:59:51|| || open || off || 75  || 0.1 flow rate, EM 2.82 kV , CATH 3.37kV(-50V), CAEN translator is used&lt;br /&gt;
|-&lt;br /&gt;
|7356|| 08/18/14 ||  20:03:05|| 20:07:58 || || open || on || 2k  || 0.1 flow rate, noise measurement&lt;br /&gt;
|-&lt;br /&gt;
|7357|| 08/18/14 ||  20:08:43 || 22:48:22 |||| open || on || 142  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7358|| 08/18-19/14 ||  22:53:13 || 10:52:44|| || open || on || 0.0082  || 0.1 flow rate , triple coincidence&lt;br /&gt;
|-&lt;br /&gt;
|7359|| 08/19/14 ||  10:55:49|| 10:59:52 || || open || on || 2.1k  || 0.1 flow rate , noise measurement&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7360|| 08/19/14 ||  11:00:38|| 14:26:38|| || open || on ||  156|| 0.1 flow rate  noise measurement with  1 Hz sampling&lt;br /&gt;
|-&lt;br /&gt;
|7361|| 08/19/14 ||  14:40:49||18:25:00 || open || on || 0 || 0.1 flow rate  with  1 Hz sampling (AND gate)&lt;br /&gt;
|-&lt;br /&gt;
|7362|| 08/19/14 ||  18:33:15||  18:38:54|| ||open || on ||1.5k  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7363|| 08/19-20/14 ||  18:39:46||  13:39:45|| ||open || on ||0.0081  || 0.1 flow rate triple coinc.(OR)&lt;br /&gt;
|-&lt;br /&gt;
|7364|| 08/20/14 ||  13:44:56|| 13:50:57 ||  ||open || off || 1.55k  || 0.1 flow rate noise measurements, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7367|| 08/20/14 ||  15:08:27 || 16:49:37 ||  ||open || off || 86  || 0.1 flow rate, 2.87, 3.42kV for GEM and CATH&lt;br /&gt;
|-&lt;br /&gt;
|7368|| 08/20/14 ||  16:53:42||  17:15:49||  ||open || on || 154  || 0.1 flow rate&lt;br /&gt;
|-&lt;br /&gt;
|7369|| 08/20/14 ||  17:17:39|| 20:28:43||  ||open || off || 86  || 0.1 flow rate, spec. amplifier decreased from 100 to 50 &lt;br /&gt;
|-&lt;br /&gt;
|7479|| 08/27/14 ||  10:02:21|| 10:42:09||  ||open || on || 64  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7480|| 08/27/14 ||  10:46:18||  14:17:22 || ||open || off || 11  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7481|| 08/27/14 ||  14:19:33 || 14:43:39 || ||close || on || 78  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7488|| 08/27/14 ||  16:16:37 || 16:48:53  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|-&lt;br /&gt;
|7491|| 08/27/14 ||  18:09:27 || 18:59:05  || || open|| on || 86  || 0.1 flow rate,&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Peak sensing measurements by 08/28/14==&lt;br /&gt;
&lt;br /&gt;
Peak sensning measurements for GEM were recorded in the time between 8:00 am to 9:44am for shutter open as the following &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Source On|| Source Off &lt;br /&gt;
|-&lt;br /&gt;
|7507 || 7506&lt;br /&gt;
|-&lt;br /&gt;
|7509 || 7508&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7511 || 7510&lt;br /&gt;
|-&lt;br /&gt;
|7513 || 7512&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7515 || 7514&lt;br /&gt;
|-&lt;br /&gt;
|7517 || 7516&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|7519 || 7518&lt;br /&gt;
|-&lt;br /&gt;
|7521 || 7520&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:unknownbootle_measurements_06_13.png | 300px]][[File:unknownbootle_measurements_14_21.png | 300px ]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Different output for each run when Peak sensing is used to measure the charge, what is noticed that the charge is different from one  run to another, but all the runs show that the amount of charge collected is bigger when the shutter is open with the source on it except for run 7511. By comparing all the runs, As the shutter is open, the maximum charge is collected by channel number 800, as the source is on the detector, the collected charge reached up to channel 1000 at most.&lt;br /&gt;
&lt;br /&gt;
Measuring the data started by 8 am, the noise rate increased so it increased the event rate from 30s to 80s event/s, and it did not decrease until now (Thur. 15:36 08/28/14). all module wiring were checked but without any result. I am using the 90/10 Ar/CO2 bottle as hope to take some measurements but when the noise level goes down maybe this evening to repeat the same measuremnts.&lt;br /&gt;
&lt;br /&gt;
The following reference shows a change in collected charge as the tenperature changes &amp;lt;ref&amp;gt;&amp;quot;Discrimination of nuclear recoils from alpha particles with superheated liquids&amp;quot; F Aubin et al 2008 New J. Phys. 10 103017 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:temp_signal_effect.jpg | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Flow rate and figures=&lt;br /&gt;
&lt;br /&gt;
;03 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 03_sourceOn.png | 450 px]]&lt;br /&gt;
[[File: 03_sourceoff.png | 450 px]]&lt;br /&gt;
[[File: 03_openOn_off_sub.png | 450 px]]&lt;br /&gt;
;02 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 02_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:02_sourceoff.png | 150 px]]&lt;br /&gt;
[[File: 02_openOn_off_sub.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
01 flow rate&lt;br /&gt;
&lt;br /&gt;
[[File: 01_sourceOn.png | 150 px]]&lt;br /&gt;
[[File:01_sourceoff.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
= Common Start Common Stop exchange=&lt;br /&gt;
&lt;br /&gt;
Edit the file &lt;br /&gt;
&lt;br /&gt;
cd /usr/local/coda/2.5/readoutlist/v1495trigPAT/&lt;br /&gt;
&lt;br /&gt;
as the following:&lt;br /&gt;
 &lt;br /&gt;
for common start comment:&lt;br /&gt;
 /* c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
for common stop uncomment:&lt;br /&gt;
  c775CommonStop(TDC_ID);&lt;br /&gt;
&lt;br /&gt;
=Ionization xsections for different particles emitted from U-233= &lt;br /&gt;
&lt;br /&gt;
; Photons&lt;br /&gt;
&lt;br /&gt;
[[File: photoabosorption_Ar.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_CO2.png | 150 px]]&lt;br /&gt;
[[File: photoabosorption_Ar_CO2.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. : http://physics.nist.gov/PhysRefData/Xcom/html/xcom1.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Electrons&lt;br /&gt;
&lt;br /&gt;
[[File: electron_ion_Ar.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75  [[File: electron_ionization_Ar.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Alpha Particles&lt;br /&gt;
&lt;br /&gt;
[[File: alpha_ionization.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
Ref. :&lt;br /&gt;
&lt;br /&gt;
http://www.exphys.jku.at/Kshells/&lt;br /&gt;
&lt;br /&gt;
Data Nucl. Data Tables 54 (1993) 75&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for GEM and the Plastic scintillator= &lt;br /&gt;
&lt;br /&gt;
;Coincidence Measurement for the scintillator PMT's without shielding and without source&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || No. of Counts (counts)||  Count rate (counts/min) &lt;br /&gt;
|-&lt;br /&gt;
|07/09/14 || 1066 || 659005 || 618&lt;br /&gt;
|-&lt;br /&gt;
|07/10/14 || 538 || 368974 || 686&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;Triple coincidence Measurement for the scintillator PMT's shielded and without source&lt;br /&gt;
&lt;br /&gt;
Triple coincidence among the 2 PMT's and the GEM detector is measured using coincidence module caberra 2144 and ortec 778 counter, count rate is 0.3+_ 0.03 Hz. However, the rate was zero before shielding.&lt;br /&gt;
&lt;br /&gt;
The following pics show The GEM output with triple coincidence signal, it is observed that different GEM peaks coincide with the triple signal, which shows that adding the shielding contaminates the neutron signal.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: GEM_triple_smallpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_bigpeak.png | 150 px]]&lt;br /&gt;
[[File: GEM_triple_twopeaks.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
=Coincidence Measurements for the Plastic scintillator after shielding= &lt;br /&gt;
&lt;br /&gt;
; Without source&lt;br /&gt;
&lt;br /&gt;
The plastic scintillator count rate before shielding and without source was in average 12 +_ 1 Hz, lead is added to the GEM and to the plastic scintillator which did not change the rate of the coincidence for the plastic scintillator  . Neither closing  the box door with lead nor adding lead to the top of the box  did  make any change in the number of counts for the plastic scintillator.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;With a source&lt;br /&gt;
&lt;br /&gt;
=Background count rate=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Date || Time || PSD_e (counts)||  PSD_e (counts/min) || LED (low disctrinimation)(counts)||LED (low disctrinimation)(counts/min)||  LED (high disctrinimation) (counts)||  LED (high disctrinimation) (counts/min)&lt;br /&gt;
|-&lt;br /&gt;
|07/01/14 || 1166 || 56671 ||  49 || 2936748 || 2519 || 10 || 0.009&lt;br /&gt;
|- &lt;br /&gt;
|07/01/14 || 231 || 10529 ||   || 572657 ||  || 1542 || &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= data graphs=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{HLE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: B_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph represents the change in the count rate of B_p, as the shutter is open (green) and as it is closed (red), the error bars get smaller since each point represents the average of two sets of daily measurements, in addition to, changing the PS discriminator's level after the second measurement.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;&amp;lt;math&amp;gt;S_{PSD}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File: S_pdaily_counts.png | 150 px]]&lt;br /&gt;
&lt;br /&gt;
The above graph has the same legend as the one for B_p, error bars increase for some data when the shutter is open, since one or more of the daily measurements has a higher number of counts because of U-233(4)'s spentaneous fission. (the number of counts is close to the number of counts as the shutter is open and the source is on).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 Small=&amp;lt;math&amp;gt;S_{PSD} - S_{PSDE}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Testing GEM Experiment  test 10/23/13=&lt;br /&gt;
&lt;br /&gt;
The GEM detector was tested for signal and discharge as the voltage of the cathode and HV-circuit divider is 3.3 kV and 2.7 kV successively.&lt;br /&gt;
&lt;br /&gt;
The GEM detector signal is observed as it used to work before. the pictures below show the signal detected as the shutter is open and as it is close.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close ||  [[File: GEM_close_1.png | 40 px]]|| [[File: GEM_close_2.png | 40 px]] &lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_1.png | 40 px ]]|| [[File: GEM_open_2.png | 40 px]] || [[File: GEM_open_3.png | 40 px]]|| [[File: GEM_open_4.png | 40 px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=THGEM#9 Counting Experiment  test 1/4/13=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[THGEM#9 Counting Experiment]]&lt;br /&gt;
&lt;br /&gt;
=GEM HV-divider circuit=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GEM HV-divider circuit in shown in the figure, measurements were recorded for for top and bottom voltage of each preamplifier. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;[[Image:GEM_HV_Dist_Net.jpg | 100px]]&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The table below shows value of the voltage on each  preamplifier's side relative to ground.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt; V_{source} \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G1T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G1B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_1 \pm 1 &amp;lt;/math&amp;gt;  || &amp;lt;math&amp;gt; V_{G2T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G2B} \pm 1 &amp;lt;/math&amp;gt;|| &amp;lt;math&amp;gt; \Delta V_2 \pm 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3T} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; V_{G3B} \pm 1 &amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \Delta V_3 \pm 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| 2550 || 2579 ||  2259 ||304 || 1671|| 1394 || 279 ||  818|| 570 ||245  &lt;br /&gt;
|- &lt;br /&gt;
| 2600 || 2630 ||  2303 ||310 || 1704|| 1421 || 285 ||834|| 581 || 250&lt;br /&gt;
|- &lt;br /&gt;
| 2650 || 2680 || 2348 || 316|| 1737||  1449  || 290 || 850|| 592 || 255&lt;br /&gt;
|- &lt;br /&gt;
| 2700 || 2731 || 2393 ||322 || 1770|| 1476 ||296 ||866|| 603 || 260&lt;br /&gt;
|- &lt;br /&gt;
| 2750 || 2781 ||  2373|| 328 || 1803|| 1503 || 302 ||882|| 614 ||264 &lt;br /&gt;
|- &lt;br /&gt;
| 2800 || 2832 ||  2482|| 332 || 1836|| 1530|| 307 || 898|| 625 || 269&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The source voltage means the voltage value on the 4-channel CAEN N470 display. (suppose to be equal to the voltage of the top GEM1).&lt;br /&gt;
&lt;br /&gt;
the values are going to be an input for ANSYS which is going to simulate the electric field for each source voltage separately,  ANSYS' output files will be an input for Garfield to simulate the electron multiplication by the triple GEM.&lt;br /&gt;
&lt;br /&gt;
= GEM alpha-Beta detector counter=&lt;br /&gt;
[[GEM Alpha-Beta detector counter]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration in LDS=&lt;br /&gt;
&lt;br /&gt;
==GEM Detector==&lt;br /&gt;
&lt;br /&gt;
[[GEM performance QDC data graphs]]&lt;br /&gt;
&lt;br /&gt;
[[Calibrating GEM detector]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:LDS_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==GEM Detector and Scintillator==&lt;br /&gt;
&lt;br /&gt;
[[GEM and Sci. data and measuurements]]&lt;br /&gt;
&lt;br /&gt;
=GEM gain data graphs and GEM Calibration at the IAC=&lt;br /&gt;
&lt;br /&gt;
 Haitham may only alter the QDC's dual timer and a CFD for the QDC in the IAC DAQ.&lt;br /&gt;
&lt;br /&gt;
 Haitham may only add signals to the NIM-&amp;gt;ECL translator&lt;br /&gt;
&lt;br /&gt;
 Haitham is not allowed to change any cables that are used for the PAA setup&lt;br /&gt;
&lt;br /&gt;
;Summary&lt;br /&gt;
&lt;br /&gt;
The detector is installed in the IAC after modifications took place in the detector design.&lt;br /&gt;
&lt;br /&gt;
These modifications are:&lt;br /&gt;
&lt;br /&gt;
1- The detector kipton window's area  increased to the same size of the GEM cards( 10X10 cm)&lt;br /&gt;
&lt;br /&gt;
2- The distance of the cathode from the first GEM increased up to 1.2 cm. previously the distance was about 3.5 mm. (No change in GEM's distances 2.8mm, or the readout 0.5 mm)&lt;br /&gt;
&lt;br /&gt;
Increasing the drift distance demands an increase in cathode potential to maintain the same values of the electric field in the old setup.&lt;br /&gt;
&lt;br /&gt;
3- The detector is installed in a wooden box, in addition to a plastic scintillator which was placed to cover part of the detector window.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[GEM performance data graphs]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Electronics Flow Chart==&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_electronics_flow_chart.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:IAC_n.png |200px]]&lt;br /&gt;
&lt;br /&gt;
=U-233 fission x-section data and fission yield=&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxsection_0.01-100MeV.gif |200px]]&lt;br /&gt;
[[File:U-233_fissionxsection_fullenergyrange.gif |200px]]&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_fissionxyield_percent.png |200px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== What is the energy distribution of Beta, Photon and alpha from U-233==&lt;br /&gt;
&lt;br /&gt;
===Alpha ===&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy (MeV)&lt;br /&gt;
|-&lt;br /&gt;
| Pb-213  || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 8.4&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Bi-213 || 5.9 &lt;br /&gt;
|-&lt;br /&gt;
|At-217 ||6.3  &lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 6.3&lt;br /&gt;
|-&lt;br /&gt;
|Th-229 ||  &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;4.85 &amp;lt;/span&amp;gt; (alpha spectrum, highest counts for is 4.85 MeV)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===Gamma===&lt;br /&gt;
&lt;br /&gt;
Gamma distribution for U-233 and its daughters are in metioned in details in the documents , [[File:u233_day_gamma.pdf]] &amp;lt;ref&amp;gt;http://www.radiochemistry.org/periodictable/gamma_spectra , Wed. 04/10/2013&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The energy range of the emitted gamma is shown in the following table .&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| nuclide || Energy Minimum || Energy Maximum (keV)&lt;br /&gt;
|-|&lt;br /&gt;
| U-233  || 25 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt; 1,119&amp;lt;/span&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
| Ra-225 || 40 || 40&lt;br /&gt;
|-&lt;br /&gt;
|Ac-225 || &amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;10.5 &amp;lt;/span&amp;gt; || 758.9&lt;br /&gt;
|-&lt;br /&gt;
|Fr-221 || 96.8 || 410.7&lt;br /&gt;
|-&lt;br /&gt;
|At-217 || 140 || 593.1&lt;br /&gt;
|-&lt;br /&gt;
|Bi-213 || 323.81 || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1,119.4 &amp;lt;/span&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Beta===&lt;br /&gt;
 &lt;br /&gt;
Beta particles are  emitted mainly from U-233 daughters as shown in the figure &amp;lt;ref&amp;gt; http://itu.jrc.ec.europa.eu/index.php?id=204, Wed. 04/10/2013 &amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[File:U-233_decay_beta_energy.jpg |200px]]&lt;br /&gt;
&lt;br /&gt;
U-233 -&amp;gt; Th-229, emitted alpha particles have energy of 4.8 MeV. &lt;br /&gt;
&lt;br /&gt;
 Insert energy distribution for Betas&lt;br /&gt;
&lt;br /&gt;
The following table shows the negative beta emitter nuclides,their parent nuclides, and  their half lives:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
|Nuclides || energy (MeV) || half life&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;Ra^{225} \rightarrow Ac^{225}&amp;lt;/math&amp;gt; ||&amp;lt;span style=&amp;quot;color:green&amp;quot;&amp;gt;0.357 &amp;lt;/span&amp;gt; || 14d.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{213} \rightarrow Po^{213}&amp;lt;/math&amp;gt; || 1.426 || 46min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Tl^{209} \rightarrow Pb^{209}&amp;lt;/math&amp;gt; || &amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;1.981 &amp;lt;/span&amp;gt; || 2.2 min.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Pb^{209} \rightarrow Bi^{209}&amp;lt;/math&amp;gt; || 0.644 || 3.25h &lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;Bi^{209}&amp;lt;/math&amp;gt; || 1.893 || stable&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==What is the energy distribution after the 1 mm FR4 shutter==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== electron shutter penetration===&lt;br /&gt;
&lt;br /&gt;
The energy distribution below represents the incidence electron on a 1 mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
[[File:E_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
 graph of electron energy for electron penetrating shutter (did any not penetrate?, how many?)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 photons below were produced by above incident electron?&lt;br /&gt;
The energy distribution of photons was observed on the opposite side of the shutter&lt;br /&gt;
&lt;br /&gt;
[[File:Photon_spectrum.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Electrons (with least energy from U-233= 0.2 MeV) pass through the shutter have the energy distribution below.&lt;br /&gt;
&lt;br /&gt;
===alpha shutter penetration===&lt;br /&gt;
&lt;br /&gt;
===photons===&lt;br /&gt;
&lt;br /&gt;
== Number of ions produced from Beta and Photon in ArCo2==&lt;br /&gt;
&lt;br /&gt;
EMTest10 is used to calculate the average number of ions (electrons) when a 101 beta of 1 MeV are fired in a world that contains ArCO2. (13.5 per primary electron).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:SecondaryElectron_Energy_1Mevbeta.png |90 px]]&lt;br /&gt;
&lt;br /&gt;
= The needed time  to observe the GEM signal=&lt;br /&gt;
&lt;br /&gt;
In the case of triple GEM detector with a gas flow of 0.3 SCFH and 2650V and 2950V on GEM cards and cathode successively, a signal lower than the noise (of 16 mV and amplified twice) is observed at 770.0s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
The normal rate (8 MHz +/- 2 as measured by the oscilloscope) is observed after 952.9s +/- 0.1.&lt;br /&gt;
&lt;br /&gt;
=THGEM card tasks and tests=&lt;br /&gt;
&lt;br /&gt;
;New THGEM cards:&lt;br /&gt;
&lt;br /&gt;
Two new fully machined cards are going to be tested in air and ArCH4, if they passes 2000 V potential bwtween the top and the bottom, then they are going to be installed in ArCh4 gas chamber.&lt;br /&gt;
&lt;br /&gt;
The older THGEM cards will have a high voltage enough to have one spark/min to clean impurities or surface defects.&lt;br /&gt;
&lt;br /&gt;
=GEM Signal after the latest modification on the fission chamber 07/01/13=&lt;br /&gt;
&lt;br /&gt;
The signal of the detector is observed as the shutter is open and close.&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| shutter close || [[File: GEM_close.jpg | 40 px]]|| [[File: GEM_close1.jpg | 40 px]]|| [[File: GEM_close2.jpg | 40 px]] || [[File: GEM_open.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
| shutter open || [[ File:GEM_open_7_1.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=GEM's signal testing when it a long cable is used=&lt;br /&gt;
&lt;br /&gt;
The GEM signal is tested when a long cable is used to transfer the signal to the oscilloscope as the shutter is open, and without the cable. Oscilloscope pictures shows an attenuation to the signal up to 30%.&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Long bnc cable|| [[File: GEM_longcable1.jpg | 40 px]]|| [[File: GEM_longcable2.jpg | 40 px]]&lt;br /&gt;
|-&lt;br /&gt;
|  Short bnc cable|| [[ File:GEM_shortcable.jpg | 40 px ]]&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Roy's detector infomation and measurements=&lt;br /&gt;
&lt;br /&gt;
U-233 metal deposited source is measured by Protean Instrument corporation gaseous detector, has a model number of WPC9450 (serial number: 0915723)and uses (P10) gas mixture, as shown below:&lt;br /&gt;
 &lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| Shutter position || Alpha particles /min.|| Beta particles /min.&lt;br /&gt;
|-&lt;br /&gt;
|  Open || 6879 || 900&lt;br /&gt;
|-&lt;br /&gt;
| Close || 1 || 38&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The source was in a plate of a diameter of 16 cm which was exposed to to the sensitive part of the detector of a height of 2-3 mm.&lt;br /&gt;
&lt;br /&gt;
The activity  of the source is calculated based on the solid angle &amp;lt;math&amp;gt; \frac {A \times W}{4\pi} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where '''A''' is the count per second&lt;br /&gt;
and '''W''' is the detector solid angle.&lt;br /&gt;
&lt;br /&gt;
For the previous measurement, the solid angle is almost &amp;lt;math&amp;gt;2\pi &amp;lt;/math&amp;gt;, so the the actvity of the source is twice the measured value in count/second.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=IAC experiment producing neutrons=&lt;br /&gt;
&lt;br /&gt;
One of the IAC experiments produces neutrons, the neutron spectrum from Tungsten target  is simulated  outside and inside water (moderator) as shown in the figure below&lt;br /&gt;
&lt;br /&gt;
[[File:moderator_nspect.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
In the simulation above , They are interested in close distances to the Tungsten target inside the water container, it is 1 ft cubed container and is made of aluminium and covered polyester.&lt;br /&gt;
&lt;br /&gt;
[[File:exp_setup.png | 70 px]]&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==THGEM design==&lt;br /&gt;
&lt;br /&gt;
THGEM#9&lt;br /&gt;
&lt;br /&gt;
[[Media:Shalem_MSthesis_march2005.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:Raz_Alon_MSthesis_Dec2007.pdf]]&lt;br /&gt;
&lt;br /&gt;
==Electric field Simulation==&lt;br /&gt;
&lt;br /&gt;
;Rim size dependence &lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_Efield_simulation.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;2010 THGEM design(s):&lt;br /&gt;
&lt;br /&gt;
[[ file: THGEM_2009_design_gas_efficiency.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Simulations_of_Particle_Interactions_with_Matter]]&lt;br /&gt;
&lt;br /&gt;
 Voss and 3 russian references for Dy(n,x) cross sections&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/abs/0903.3819 Dy photon gammas spectrum&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ippe.obninsk.ru/podr/cjd/kobra13.php?SubentID=30974002&lt;br /&gt;
&lt;br /&gt;
http://www.americanelements.com/thoxst.html&lt;br /&gt;
&lt;br /&gt;
http://arxiv.org/pdf/physics/0404119&lt;br /&gt;
&lt;br /&gt;
NIM_A535_2004_93[http://wiki.iac.isu.edu/index.php/Image:Detectors_for_energy-resolved_fast_neutron_imaging.PDF#filehistory]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Image:NIM_A590_2008_pg134_Eberhardt.pdf]]  Prep Targets&lt;br /&gt;
&lt;br /&gt;
Neutron cross sections for different elements [[Media:Neutron_cross_sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www-nds.iaea.org/RIPL-2/&lt;br /&gt;
&lt;br /&gt;
[[Media:n gamma cross sections at 25 keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n alpha cross section at 14.2 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:ne cross section at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:high enegy fission x-section.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:N_gamma_x-section_at_400_keV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:x-sections of  reactions at 14 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media:n p x-section at 14.3MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 14.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: elastic x-section at 0.5 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n gamma x-section at 1 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
[[Media: n 2n x-section at 14.3 MeV.jpg]]&lt;br /&gt;
&lt;br /&gt;
Donald James Hughes, Neutron cross sections, 2nd edition 1958, u.s.a atomic energy commission.[[Media:Neutron cross sections.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Image:NSAE_ 151_ 2005_ 319-334_ Y.D. Lee.pdf]]&lt;br /&gt;
&lt;br /&gt;
TGEM-2009 [[File:TGEM_2009.pdf]]&lt;br /&gt;
&lt;br /&gt;
12 Volt power supply system.&lt;br /&gt;
&lt;br /&gt;
http://www.lnf.infn.it/esperimenti/imagem/doc/NIMA_46128.pdf&lt;br /&gt;
&lt;br /&gt;
http://electrontube.com.[[Media: rp097mono HV divier.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm#anchor550078&lt;br /&gt;
&lt;br /&gt;
http://en.wikipedia.org/wiki/PC_board&lt;br /&gt;
&lt;br /&gt;
http://wikipedia.org&lt;br /&gt;
&lt;br /&gt;
[http://arxiv.org/abs/0807.2026 A : concise review on THGEM detectors A.Breskin, R. Alon, M. Cortesi, R. Chechik, J. Miyamoto, V. Dangendorf, J. Maia, J. M. F. Dos Santos]&lt;br /&gt;
&lt;br /&gt;
GEANT4_Paticles_Models[http://geant4.cern.ch/support/proc_mod_catalog/index.shtml]&lt;br /&gt;
&lt;br /&gt;
Resistors online store : http://www.justradios.com/rescart.html&lt;br /&gt;
&lt;br /&gt;
==RETGEMs==&lt;br /&gt;
&lt;br /&gt;
[[Media:Jinst8_02_p02012_THGEM_spark.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media:2010_INST_5_P03002.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
;Thick GEM COBRA:&lt;br /&gt;
&lt;br /&gt;
[[Media:THGEM_COBRA_08_10.pdf‎]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Media: Nucl_Phys_B_Bidault_ novel UV photon detector.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Mauro micro pattern gaseuos detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[Media:Development and First Tests of GEM-Like Detectors With Resistive Electrodes.pdf]]&lt;br /&gt;
&lt;br /&gt;
http://www.supplydivision.co.uk/genitem.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.radioshack.com/search/index.jsp?kwCatId=&amp;amp;kw=24%20gauge%20wires&amp;amp;origkw=24%20gauge%20wires&amp;amp;sr=1&lt;br /&gt;
&lt;br /&gt;
Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors (HV circuit)[http://wiki.iac.isu.edu/index.php/File:Media-Thick_GEM_versus_thin_GEM_in_two_phase_argon_avalanche_detectors_(HV_circuit).pdf#filelinks]&lt;br /&gt;
&lt;br /&gt;
Stainless Steel deflection [http://www.bssa.org.uk/topics.php?article=126]&lt;br /&gt;
&lt;br /&gt;
==Data Sheets==&lt;br /&gt;
&lt;br /&gt;
radioactive surface cleaner NoCount MDSD [[File:radioactive_surface_cleaner.pdf]].&lt;br /&gt;
&lt;br /&gt;
==Th-Xsection references==&lt;br /&gt;
[[File:Th-232_fxsection_Behrens_0.7-1.4MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Blons_1975_1.2-1.8MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_ermagambetov_0-3MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Henkel_0-9MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_Ohsawa_original.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_pankratov_3-35MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_protopopov_distancefromthesource.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:Th-232_fxsection_rago_12.5-18MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
==U-238-Xsection and coating references==&lt;br /&gt;
&lt;br /&gt;
relative cross section and calibration samples characteristics for a well determined number of fissions per second&lt;br /&gt;
&lt;br /&gt;
[[File:Eismont_relative_absolute_nf_induced_ intermediate energy.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;U_238 cross section error analysis: &lt;br /&gt;
&lt;br /&gt;
INTERNATIONAL EVALUATION OF NEUTRON CROSS-SECTION STANDARDS, INTERNATIONAL ATOMIC ENERGY AGENCY,VIENNA, 2007 [[File:U238-xsection.pdf]]&lt;br /&gt;
&lt;br /&gt;
U_238 (0.5-4MeV) and Th_232 (1-6MeV) fission cross section with statistical error.[[File:Th-232_U238_xsetion_data_ebars.txt]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Pankratov_fxsection_Th232_U233_U235_Np237_U238_5-37MeV.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Thorium Coating==&lt;br /&gt;
ThF4 target for sputtering coatings&lt;br /&gt;
&lt;br /&gt;
http://www.cerac.com/pubs/proddata/thf4.htm&lt;br /&gt;
&lt;br /&gt;
==Machining Uranium==&lt;br /&gt;
&lt;br /&gt;
Uranium will ignite in powder form&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.springerlink.com/content/rr072r52163x0833/&lt;br /&gt;
&lt;br /&gt;
;coating Uranium&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVV-46G57SW-53&amp;amp;_user=10&amp;amp;_coverDate=10%2F01%2F1991&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1388383717&amp;amp;_rerunOrigin=google&amp;amp;_acct=C000050221&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=10&amp;amp;md5=c3229e061695dfa28617f9f5db1ef55d]]&lt;br /&gt;
&lt;br /&gt;
http://cat.inist.fr/?aModele=afficheN&amp;amp;cpsidt=16864172&lt;br /&gt;
&lt;br /&gt;
Calorimeters/Detectors:&lt;br /&gt;
DU sheet is in wide-scale use as an absorber material in high-energy physics research at large accelerator laboratories. The high atomic number and density of DU presents a large number of atoms per unit volume to interact with the particles emerging from collisions in these detectors. Also the slight background radiation from DU enables in situ calibration of the electronic read out devices within such detectors, thereby improving the accuracy of measurement. &lt;br /&gt;
&lt;br /&gt;
http://www.2spi.com/catalog/chem/depleted-uranium-products.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[http://books.google.com/books?id=NRXnXmFRjWYC&amp;amp;pg=SA48-PA17&amp;amp;lpg=SA48-PA17&amp;amp;dq=depleted+uranium+coating&amp;amp;source=bl&amp;amp;ots=a6jHsdI6Ec&amp;amp;sig=zVxKGeD4E42gAVkr8Otg9bfpkyg&amp;amp;hl=en&amp;amp;ei=8FgtTIH1HMGC8gbNl-S-Aw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=6&amp;amp;ved=0CCoQ6AEwBThG]&lt;br /&gt;
&lt;br /&gt;
[http://www.google.com/url?sa=t&amp;amp;source=web&amp;amp;cd=90&amp;amp;ved=0CDYQFjAJOFA&amp;amp;url=http%3A%2F%2Fwww.ga.com%2Fenergy%2Ffiles%2FIFT_Catalog.pdf&amp;amp;ei=RFktTPbgKYL88AbC1tSSAw&amp;amp;usg=AFQjCNE3VbqBWbvcKln4pJVAj8FyKfcOig]&lt;br /&gt;
&lt;br /&gt;
;IAEA Photonuclear Data Library  [http://www-nds.iaea.org/photonuclear/]&lt;br /&gt;
&lt;br /&gt;
;Data Acquisition &lt;br /&gt;
&lt;br /&gt;
Warren_logbook[http://wiki.iac.isu.edu/index.php/Warren_Parsons_Log_Book]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Warren_Thesis [http://wiki.iac.isu.edu/index.php/Warren_Parsons_MS_Thesis]&lt;br /&gt;
&lt;br /&gt;
=Related To Gaseous Detectors=&lt;br /&gt;
&lt;br /&gt;
==Breakdown and Detector Failure  (10/21/10)==&lt;br /&gt;
&lt;br /&gt;
;Different kind of micro-pattern detectors&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
;References&lt;br /&gt;
&lt;br /&gt;
1- A. Bressan, M. Hocha : NIM A 424 (1999) 321—342 [[File:High_rate_behavior_and_discharge_limits_in micro-pattern_detectors .pdf]]&lt;br /&gt;
&lt;br /&gt;
2- Fonte and Peskov IEEE 1999 :[[File:fundamental_limitations_of_high_rate_gaseous_detectors.pdf]]&lt;br /&gt;
&lt;br /&gt;
3- B. Schmidt: NIM A 419 (1998) 230—238 [[File:Microstrip_gas_chambers_Recent_developments_radiation_damage.pdf]]&lt;br /&gt;
&lt;br /&gt;
= Ideas=&lt;br /&gt;
&lt;br /&gt;
1.) Can we mix resistive paste (Encre MINICO) with TH-232.  We construct a &amp;quot;bed of nails&amp;quot; to place a predrilled G-10 board with a copper border.  The nails fill in the holes of the G-10 to keep the paste out.  Ecre MINICO is a resistive paste used for transistors.&lt;br /&gt;
&lt;br /&gt;
a.) Get some resistive paste.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.leggesystems.com/p-253-elimstat-uxm-ccp.aspx&lt;br /&gt;
&lt;br /&gt;
Resistive glue to compare&lt;br /&gt;
&lt;br /&gt;
[[File:Duralco_4461.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/conformal.html?tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=764&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://www.ellsworth.com/display/productdetail.html?productid=2067&amp;amp;Tab=Products&lt;br /&gt;
&lt;br /&gt;
http://www.cotronics.com/vo/cotr/ea_electricalresistant.htm&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
b.) mix with a metal similar to Th-232.&lt;br /&gt;
&lt;br /&gt;
c.) construct bed of 0.4 mm nails. Look for 0.4 mm diameter pins.&lt;br /&gt;
&lt;br /&gt;
==7/31/2009==&lt;br /&gt;
New vendor for carbon paste.&lt;br /&gt;
&lt;br /&gt;
http://www.electrapolymers.com/productItem.asp?id=33&lt;br /&gt;
&lt;br /&gt;
The data sheet does not show any information about the thickness of the paste.&lt;br /&gt;
&lt;br /&gt;
The company has a distributor in the usa (877)-867-9668. A phone call is expected on Sat. 8/3/2009 about the availability of the product.&lt;br /&gt;
&lt;br /&gt;
= TGEM Mask Design=&lt;br /&gt;
&lt;br /&gt;
Coating U-238 or Th-232 is essential for neutron detection in the range 2-14 MeV, but THGEM contains holes that should be protected from any coating material. So, a mask is designed to cover these holes. The holes are in drilled to be on the corners of hexagonal of 1mm side length as in the figure:&lt;br /&gt;
&lt;br /&gt;
[[Image: hexagonal _representaion_holes_04mm_1mmc2c.jpg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The mask is made of stainless steel, 10 um laser tolerance with cut the plate to get the shape in the figure: &lt;br /&gt;
&lt;br /&gt;
[[Image: holes_covered_by_mask.jpeg | 300 px]]&lt;br /&gt;
&lt;br /&gt;
Please look at the following files for more details:&lt;br /&gt;
&lt;br /&gt;
Make number bold black font.  Add color so it is clear that they are holes in a material.&lt;br /&gt;
&lt;br /&gt;
[[File:copper_foil_04mm.pdf]]&lt;br /&gt;
&lt;br /&gt;
[[File:holes_mask_together.pdf]]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
[[TGEM_Mask_Design]]&lt;br /&gt;
&lt;br /&gt;
=P_D=&lt;br /&gt;
&lt;br /&gt;
[[Performance of THGEM as a Neutron Detector]]&lt;br /&gt;
&lt;br /&gt;
[[H_Proposal_Defense]]&lt;br /&gt;
&lt;br /&gt;
=Vendor=&lt;br /&gt;
===Thick Film Screen Printers===&lt;br /&gt;
&lt;br /&gt;
http://www.sciquip.com/browses/browse_Cat.asp?Category=Screen+Printers&lt;br /&gt;
&lt;br /&gt;
http://www.marubeni-sunnyvale.com/screen_printing.html&lt;br /&gt;
&lt;br /&gt;
[http://wiki.iac.isu.edu/index.php/TGEMS Go Back] [[TGEMS]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===tektronix oscilloscope===&lt;br /&gt;
&lt;br /&gt;
134.50.3.73&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
http://134.50.203.63/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;references/&amp;gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Beta_Transmission_and_Ionization&amp;diff=100306</id>
		<title>Beta Transmission and Ionization</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Beta_Transmission_and_Ionization&amp;diff=100306"/>
		<updated>2015-04-20T03:54:35Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;GEANT4  simulated Beta particles in the drift region with a 90/10 Ar/CO2 gas. U-233 emits Beta particles with a range extends up to 600 keV, Although Beta particles are low in rates as compared to Alpha rates; they contribute in the detector total charge. GEANT4 is used for simulating the charge for a Beta particle that passed through the drift region, and estimated the primary and secondary electrons for each Beta particle energy. Additionally, GEANT4 helps studying the penetration of beta particles through 1mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
= Beta particles energy rates=&lt;br /&gt;
&lt;br /&gt;
Beta particles are emitted from U-233 radioactive isotope, their energy spectrum vs the percentage of the emitted Beta is shown in figure XX. Based on the figure, the rates are lower than 0.1 percent,  with only two specific energies reach up to 6 percent for 10 keV for one of the energies, and 30 keV for the other.&lt;br /&gt;
&lt;br /&gt;
[[File: beta_energy_percentages.png  | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Primary and secondary ionization=&lt;br /&gt;
&lt;br /&gt;
A simulation for Beta ionization was performed by using GEANT4. GEANT4 simulated the interaction of a beta particle in the drift region that contained 90/10 Ar/CO2 gas; the simulation estimated the ionization primary and secondary electrons. Figure XX illustrates that the number of primary electrons is inversely proportional to the incident beta particle energy; such a relationship agrees with Bethe-Bloch equation for estimating the energy loss. The figure also shows GEANT4 underestimation for the number of primaries when for beta particle of energy of 10 keV, and when the energy is higher than 300 keV; one of the reasons that GEANT4 does not consider the minimum ionization for an ion-electron for Ar/CO2 or miscalculate it, or the electron cut is still high that makes it hard to track the low energy electrons. On the other hand, Garfield simulation for the number of electrons in the drift region when a beta particle passes through, and agreed with Bethe-Bloch formula, so the highest number of primaries is for low energy betas.Additionally, the number of primaries decreases gradually as beta energy increases to reach to the minimum ionization for Ar/CO2 gas which is in average 24 eV.  &lt;br /&gt;
&lt;br /&gt;
[[File: G4_1cmAr90CO2_Beta_primaryElecN.png| 300 px]][http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1967ApJS...14..207L&amp;amp;db_key=AST&amp;amp;page_ind=0&amp;amp;plate_select=NO&amp;amp;data_type=GIF&amp;amp;type=SCREEN_GIF&amp;amp;classic=YES]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Leo: 1 e-ion pair per 30 eV of energy loss , a 100 keV electron loosing all of its energy to ionization produces 3333 e-ion pairs&lt;br /&gt;
&lt;br /&gt;
Sauli: a 100 keV electron causes 1000 e-ion pairs per cm and 3000 secondary e-ion pairs.&lt;br /&gt;
&lt;br /&gt;
 What is GEANT4 cut that produces 1000 primary ionization.&lt;br /&gt;
&lt;br /&gt;
 Why is Garfield only getting 30&lt;br /&gt;
&lt;br /&gt;
  Why is e-star only getting 200&lt;br /&gt;
&lt;br /&gt;
G4 cut is in Em10PhysicsList.cc,  line 111, and it is a length cut, to have 10^3 primaries and 3x10^3 secondaries, range cut = 0.03 mm . which means to track to zero electrons of range of 0.03 mm.&lt;br /&gt;
&lt;br /&gt;
= Beta Ionization with FR4 shutter=&lt;br /&gt;
&lt;br /&gt;
The FR4 shutter stops the low energy betas from U-233, and passes the high energy ones to ionize the gas in the drift region. U-233 beta emission relative rate is as low as 0.1 for most beta energies, and discussed previously, the highest beta rates are for those of kinetic energy of 10 keV and 30 keV.  GEANT4 simulation shows in  figure yy  that 80 percent of Beta particles of energy of 1 MeV penetrate the shutter, and close to 100 percent penetration for beta energies which are equal or larger than 1.3 MeV. However, those low energy betas have the major contribution to the total number of primary and secondary electrons in the drift region; therefore, when the shutter is closed, only beta particles with energy more than 400keV contribute to the number of primary and secondary electrons. Those Betas have a negligible effect on the detector total charge due to the their low emission rates and the amount of charge they create in the drift region.&lt;br /&gt;
&lt;br /&gt;
[[File:e_trans_1mmFR4_keV_percent.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Combined Gamma=&lt;br /&gt;
&lt;br /&gt;
Electron multiple scattering causes Gamma particles to appear through beta transmission in the FR4. Electron scattering is one  of the interactions of beta particles with FR4, photons are produced through this process depending on beta's energy.&lt;br /&gt;
&lt;br /&gt;
[[File:e_trans_FR4_keV_gammaN.png || 300 px]]&lt;br /&gt;
&lt;br /&gt;
It is noticed from the figure above that the maximum scattering cross section is for 1100 keV beta particles, the number of photons reaches to 1800  for each beta particle that transport through 1cm of FR4.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[ HAM_Beta_extras]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
GO BACK [https://wiki.iac.isu.edu/index.php/Performance_of_THGEM_as_a_Neutron_Detector#Simulation_and_Analysis]&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:G4_1cmAr90CO2_Beta_primaryElecN.png&amp;diff=100305</id>
		<title>File:G4 1cmAr90CO2 Beta primaryElecN.png</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:G4_1cmAr90CO2_Beta_primaryElecN.png&amp;diff=100305"/>
		<updated>2015-04-20T03:24:39Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: uploaded a new version of &amp;quot;File:G4 1cmAr90CO2 Beta primaryElecN.png&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Beta_Transmission_and_Ionization&amp;diff=100304</id>
		<title>Beta Transmission and Ionization</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Beta_Transmission_and_Ionization&amp;diff=100304"/>
		<updated>2015-04-18T22:33:39Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Primary and secondary ionization */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;GEANT4  simulated Beta particles in the drift region with a 90/10 Ar/CO2 gas. U-233 emits Beta particles with a range extends up to 600 keV, Although Beta particles are low in rates as compared to Alpha rates; they contribute in the detector total charge. GEANT4 is used for simulating the charge for a Beta particle that passed through the drift region, and estimated the primary and secondary electrons for each Beta particle energy. Additionally, GEANT4 helps studying the penetration of beta particles through 1mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
= Beta particles energy rates=&lt;br /&gt;
&lt;br /&gt;
Beta particles are emitted from U-233 radioactive isotope, their energy spectrum vs the percentage of the emitted Beta is shown in figure XX. Based on the figure, the rates are lower than 0.1 percent,  with only two specific energies reach up to 6 percent for 10 keV for one of the energies, and 30 keV for the other.&lt;br /&gt;
&lt;br /&gt;
[[File: beta_energy_percentages.png  | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Primary and secondary ionization=&lt;br /&gt;
&lt;br /&gt;
A simulation for Beta ionization was performed by using GEANT4. GEANT4 simulated the interaction of a beta particle in the drift region that contained 90/10 Ar/CO2 gas; the simulation estimated the ionization primary and secondary electrons. Figure XX illustrates that the number of primary electrons is inversely proportional to the incident beta particle energy; such a relationship agrees with Bethe-Bloch equation for estimating the energy loss. The figure also shows GEANT4 underestimation for the number of primaries when for beta particle of energy of 10 keV, and when the energy is higher than 300 keV; one of the reasons that GEANT4 does not consider the minimum ionization for an ion-electron for Ar/CO2 or miscalculate it, or the electron cut is still high that makes it hard to track the low energy electrons. On the other hand, Garfield simulation for the number of electrons in the drift region when a beta particle passes through, and agreed with Bethe-Bloch formula, so the highest number of primaries is for low energy betas.Additionally, the number of primaries decreases gradually as beta energy increases to reach to the minimum ionization for Ar/CO2 gas which is in average 24 eV.  &lt;br /&gt;
&lt;br /&gt;
[[File: G4_1cmAr90CO2_Beta_primaryElecN.png| 300 px]][http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1967ApJS...14..207L&amp;amp;db_key=AST&amp;amp;page_ind=0&amp;amp;plate_select=NO&amp;amp;data_type=GIF&amp;amp;type=SCREEN_GIF&amp;amp;classic=YES]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Leo: 1 e-ion pair per 30 eV of energy loss , a 100 keV electron loosing all of its energy to ionization produces 3333 e-ion pairs&lt;br /&gt;
&lt;br /&gt;
Sauli: a 100 keV electron causes 1000 e-ion pairs per cm and 3000 secondary e-ion pairs.&lt;br /&gt;
&lt;br /&gt;
 What is GEANT4 cut that produces 1000 primary ionization.&lt;br /&gt;
&lt;br /&gt;
 Why is Garfield only getting 30&lt;br /&gt;
&lt;br /&gt;
  Why is e-star only getting 200&lt;br /&gt;
&lt;br /&gt;
G4 cut is in Em10PhysicsList.cc,  line 111, and it is a length cut, to have 10^3 primaries and 3x10^3 secondaries, range cut = 0.03 mm . which means to track to zero electrons of range of 0.03 mm.&lt;br /&gt;
&lt;br /&gt;
= Beta Ionization with FR4 shutter=&lt;br /&gt;
&lt;br /&gt;
The FR4 shutter stops the low energy betas from U-233, and passes the high energy ones to ionize the gas in the drift region. U-233 beta emission relative rate is as low as 0.1 for most beta energies, and discussed previously, the highest beta rates are for those of kinetic energy of 10 keV and 30 keV.  GEANT4 simulation shows in  figure yy  that 80 percent of Beta particles of energy of 1 MeV penetrate the shutter, and close to 100 percent penetration for beta energies which are equal or larger than 1.3 MeV. However, those low energy betas have the major contribution to the total number of primary and secondary electrons in the drift region; therefore, when the shutter is closed, only beta particles with energy more than 400keV contribute to the number of primary and secondary electrons. Those Betas have a negligible effect on the detector total charge due to the their low emission rates and the amount of charge they create in the drift region.&lt;br /&gt;
&lt;br /&gt;
[[File:e_trans_1mmFR4_keV_percent.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Combined Gamma=&lt;br /&gt;
&lt;br /&gt;
Electron multiple scattering causes Gamma particles to appear through beta transmission in the FR4. Electron scattering is one  of the interactions of beta particles with FR4, photons are produced through this process depending on beta's energy.&lt;br /&gt;
&lt;br /&gt;
[[File:e_trans_FR4_keV_gammaN.png || 300 px]]&lt;br /&gt;
&lt;br /&gt;
It is noticed from the figure above that the maximum scattering cross section is for 1100 keV beta particles, the number of photons reaches to 1800  for each beta particle that transport through 1cm of FR4.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[ HAM_Beta_extras]]&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Beta_Transmission_and_Ionization&amp;diff=100303</id>
		<title>Beta Transmission and Ionization</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Beta_Transmission_and_Ionization&amp;diff=100303"/>
		<updated>2015-04-18T22:32:03Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* Primary and secondary ionization */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;GEANT4  simulated Beta particles in the drift region with a 90/10 Ar/CO2 gas. U-233 emits Beta particles with a range extends up to 600 keV, Although Beta particles are low in rates as compared to Alpha rates; they contribute in the detector total charge. GEANT4 is used for simulating the charge for a Beta particle that passed through the drift region, and estimated the primary and secondary electrons for each Beta particle energy. Additionally, GEANT4 helps studying the penetration of beta particles through 1mm FR4 shutter.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
= Beta particles energy rates=&lt;br /&gt;
&lt;br /&gt;
Beta particles are emitted from U-233 radioactive isotope, their energy spectrum vs the percentage of the emitted Beta is shown in figure XX. Based on the figure, the rates are lower than 0.1 percent,  with only two specific energies reach up to 6 percent for 10 keV for one of the energies, and 30 keV for the other.&lt;br /&gt;
&lt;br /&gt;
[[File: beta_energy_percentages.png  | 300 px]]&lt;br /&gt;
&lt;br /&gt;
=Primary and secondary ionization=&lt;br /&gt;
&lt;br /&gt;
A simulation for Beta ionization was performed by using GEANT4. GEANT4 simulated the interaction of a beta particle in the drift region that contained 90/10 Ar/CO2 gas; the simulation estimated the ionization primary and secondary electrons. Figure XX illustrates that the number of primary electrons is inversely proportional to the incident beta particle energy; such a relationship agrees with Bethe-Bloch equation for estimating the energy loss. The figure also shows GEANT4 underestimation for the number of primaries when for beta particle of energy of 10 keV, and when the energy is higher than 300 keV; one of the reasons that GEANT4 does not consider the minimum ionization for an ion-electron for Ar/CO2 or miscalculate it, or the electron cut is still high that makes it hard to track the low energy electrons. On the other hand, Garfield simulation for the number of electrons in the drift region when a beta particle passes through, and agreed with Bethe-Bloch formula, so the highest number of primaries is for low energy betas.Additionally, the number of primaries decreases gradually as beta energy increases to reach to the minimum ionization for Ar/CO2 gas which is in average 24 eV.  &lt;br /&gt;
&lt;br /&gt;
[[File: G4_1cmAr90CO2_Beta_primaryElecN.png| 300 px]][http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1967ApJS...14..207L&amp;amp;db_key=AST&amp;amp;page_ind=0&amp;amp;plate_select=NO&amp;amp;data_type=GIF&amp;amp;type=SCREEN_GIF&amp;amp;classic=YES]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Leo: 1 e-ion pair per 30 eV of energy loss , a 100 keV electron loosing all of its energy to ionization produces 3333 e-ion pairs&lt;br /&gt;
&lt;br /&gt;
Sauli: a 100 keV electron causes 1000 e-ion pairs per cm and 3000 secondary e-ion pairs.&lt;br /&gt;
&lt;br /&gt;
 What is GEANT4 cut that produces 1000 primary ionization.&lt;br /&gt;
&lt;br /&gt;
 Why is Garfield only getting 30&lt;br /&gt;
&lt;br /&gt;
  Why is e-star only getting 200&lt;br /&gt;
&lt;br /&gt;
G4 cut is in Em10PhysicsList.cc,  line 111, and it is a length cut, to have 10^3 primaries and 3x10^3 secondaries, the cut = 0.03 mm .&lt;br /&gt;
&lt;br /&gt;
= Beta Ionization with FR4 shutter=&lt;br /&gt;
&lt;br /&gt;
The FR4 shutter stops the low energy betas from U-233, and passes the high energy ones to ionize the gas in the drift region. U-233 beta emission relative rate is as low as 0.1 for most beta energies, and discussed previously, the highest beta rates are for those of kinetic energy of 10 keV and 30 keV.  GEANT4 simulation shows in  figure yy  that 80 percent of Beta particles of energy of 1 MeV penetrate the shutter, and close to 100 percent penetration for beta energies which are equal or larger than 1.3 MeV. However, those low energy betas have the major contribution to the total number of primary and secondary electrons in the drift region; therefore, when the shutter is closed, only beta particles with energy more than 400keV contribute to the number of primary and secondary electrons. Those Betas have a negligible effect on the detector total charge due to the their low emission rates and the amount of charge they create in the drift region.&lt;br /&gt;
&lt;br /&gt;
[[File:e_trans_1mmFR4_keV_percent.png | 300px]]&lt;br /&gt;
&lt;br /&gt;
=Combined Gamma=&lt;br /&gt;
&lt;br /&gt;
Electron multiple scattering causes Gamma particles to appear through beta transmission in the FR4. Electron scattering is one  of the interactions of beta particles with FR4, photons are produced through this process depending on beta's energy.&lt;br /&gt;
&lt;br /&gt;
[[File:e_trans_FR4_keV_gammaN.png || 300 px]]&lt;br /&gt;
&lt;br /&gt;
It is noticed from the figure above that the maximum scattering cross section is for 1100 keV beta particles, the number of photons reaches to 1800  for each beta particle that transport through 1cm of FR4.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[ HAM_Beta_extras]]&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Submitted_parts_of_the_dissertation_and_their_comments&amp;diff=100302</id>
		<title>Submitted parts of the dissertation and their comments</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Submitted_parts_of_the_dissertation_and_their_comments&amp;diff=100302"/>
		<updated>2015-04-17T20:47:23Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: /* 03/26/14 */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=30/25/14=&lt;br /&gt;
&lt;br /&gt;
[[File:beginningtochapter1.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
On Thu, Mar 27, 2014 at 10:09 AM, Tony Forest &amp;lt;foretony@isu.edu&amp;gt; wrote:&lt;br /&gt;
Haitham:&lt;br /&gt;
&lt;br /&gt;
You need to include more content in Chapter 1 and reorganize it.&lt;br /&gt;
&lt;br /&gt;
You should start from the standpoint of trying to explain your work to your daughter and then end with information directed towards the Ph.D. committee.&lt;br /&gt;
&lt;br /&gt;
For example,  you should introduce the concept of ionization in the first Chapter but a detailed description of how fission fragments will produce a signal in the GEM fission chamber is presented in the Simulations chapter.  &lt;br /&gt;
&lt;br /&gt;
After describing ionization chambers and GEM foils in general you would move onto fission chambers and then neutron detection in Chapter 1.&lt;br /&gt;
&lt;br /&gt;
An introductory paragraph can lay out the contents of Chapter 1 in order to lead into the description contained in Chapter 1.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
You could move energy loss by charged particles into the Simualtion chapter.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| page number || Comments&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=04/17/14=&lt;br /&gt;
&lt;br /&gt;
[[File:detector_description.pdf]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;4&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
| page number || Comments&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=03/28/14=&lt;br /&gt;
&lt;br /&gt;
[[File:simulation.pdf ]]&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:Detector_description.pdf&amp;diff=100301</id>
		<title>File:Detector description.pdf</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:Detector_description.pdf&amp;diff=100301"/>
		<updated>2015-04-17T20:46:44Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: uploaded a new version of &amp;quot;File:Detector description.pdf&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=File:G4_1cmAr90CO2_Beta_primaryElecN.png&amp;diff=100288</id>
		<title>File:G4 1cmAr90CO2 Beta primaryElecN.png</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=File:G4_1cmAr90CO2_Beta_primaryElecN.png&amp;diff=100288"/>
		<updated>2015-04-14T19:42:21Z</updated>

		<summary type="html">&lt;p&gt;Abdehait: uploaded a new version of &amp;quot;File:G4 1cmAr90CO2 Beta primaryElecN.png&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
</feed>