Difference between revisions of "05/12/2011"
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− | Let's do the '''random coincidence cosmic ray test'''. PS1 and PS2 is about 30 cm away from each other. And let's look on the coincidence signal between PS1 and PS2: | + | Let's do the '''random coincidence cosmic ray test'''. |
+ | PS1 and PS2 is about 30 cm away from each other. And let's look on the coincidence signal between PS1 and PS2: | ||
{| border="1" cellspacing="0" style="text-align: center; width: 800px; height: 100px;" | {| border="1" cellspacing="0" style="text-align: center; width: 800px; height: 100px;" | ||
! scope="col" width="50" | | ! scope="col" width="50" | | ||
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[[File:Rnd coinc cosmic.png | 800px]] | [[File:Rnd coinc cosmic.png | 800px]] | ||
+ | |||
+ | |||
+ | Let's do the '''random coincidence cosmic ray test''' again. | ||
+ | But now the distance between PS1 and PS2 is about 5 cm. And let's look on the coincidence signal between PS1 and PS2: | ||
+ | {| border="1" cellspacing="0" style="text-align: center; width: 800px; height: 100px;" | ||
+ | ! scope="col" width="50" | | ||
+ | ! scope="col" width="50" | total counts | ||
+ | ! scope="col" width="50" | time | ||
+ | ! scope="col" width="50" | counts/min | ||
+ | ! scope="col" width="50" | counts/sec | ||
+ | |- | ||
+ | !PS1 | ||
+ | |<math>\pm101.2</math>||70 min||<math>146.4\pm1.44</math>||<math>2.44\pm0.02</math> | ||
+ | |- | ||
+ | !PS1 | ||
+ | |<math>\pm113.9</math>||70 min||<math>185.3\pm1.63</math>||<math>3.09\pm0.03</math> | ||
+ | |- | ||
+ | !PS1+PS2 | ||
+ | |<math>\pm1.7</math>||70 min||<math>0.043\pm0.024</math>||<math>0.0007\pm0.0004</math> | ||
+ | |} | ||
+ | |||
+ | |||
+ | |||
Revision as of 21:27, 12 May 2011
The powers are:
PS1 and PS2: -1000 V (the old 2-channel TENNELEC TC952) n's: -1100 V (the new 2-channel C.A.E.N N471)
The thresholds are:
PS1 and PS2: -80 mV n's: -200 mV
The discriminator widths are:
PS1: -20 ns PS2: -10 ns n's: -20 ns
Let's do the random coincidence cosmic ray test.
PS1 and PS2 is about 30 cm away from each other. And let's look on the coincidence signal between PS1 and PS2:
total counts | time | counts/min | counts/sec | |
---|---|---|---|---|
PS1 | 70 min | |||
PS1 | 70 min | |||
PS1+PS2 | 70 min |
And below my scope pictures of this rear event:
Let's do the random coincidence cosmic ray test again.
But now the distance between PS1 and PS2 is about 5 cm. And let's look on the coincidence signal between PS1 and PS2:
total counts | time | counts/min | counts/sec | |
---|---|---|---|---|
PS1 | 70 min | |||
PS1 | 70 min | |||
PS1+PS2 | 70 min |
Let's do the 2n correlation test with CF252 source. The voltages and thresholds are the same.
First the set up is like:
- PS1 and PS2 are parallel to each other and are faced to the source.
- the CF252 source in the middle
- the distance between PS1(PS2) and source is 6 cm
The total number of events (2n fission events + random coincident) are:
total counts | time | counts/min | counts/sec | |
---|---|---|---|---|
PS1 | 10 min | |||
PS1 | 10 min | |||
PS1+PS2 | 10 min |
Second the set up is like:
- PS1 and PS2 are perpendicular to each other and are faced to the source.
- the CF252 source in the middle
- the distance between PS1(PS2) and source is 6 cm
The total number of events (2n fission events + random coincident) are:
total counts | time | counts/min | counts/sec | |
---|---|---|---|---|
PS1 | 10 min | |||
PS1 | 10 min | |||
PS1+PS2 | 10 min |