Difference between revisions of "September 4, 2007 - Cosmic Telescope"
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{| border="1" cellpadding="20" cellspacing="0" | {| border="1" cellpadding="20" cellspacing="0" | ||
− | ! colspan="2"| | + | ! colspan="2"|Angular Distribution |
|- | |- | ||
|Time Start | |Time Start | ||
|Time Stop | |Time Stop | ||
− | |Time elapsed (min.) | + | |Time elapsed (min.; hour) |
|Thresholds on both Scintillators | |Thresholds on both Scintillators | ||
|Singles Count (on top) | |Singles Count (on top) | ||
|Coinc. Counts | |Coinc. Counts | ||
|Coinc. per minute | |Coinc. per minute | ||
+ | |Coinc. per Hour | ||
|Angle measure | |Angle measure | ||
|- | |- | ||
|1:35 pm on 8/31 | |1:35 pm on 8/31 | ||
|1:10 pm on 9/04 | |1:10 pm on 9/04 | ||
− | |5725 min | + | |5725 min; 95.42 hr |
|225 | |225 | ||
|626816 | |626816 | ||
|1654 | |1654 | ||
|.2889 | |.2889 | ||
+ | |17.33 | ||
|75 degrees | |75 degrees | ||
|}<br> | |}<br> | ||
+ | Cosmic rates measured each hour when the telecope accepts cosmics which intersect the earth's surface perpendicularly (defined as zero degrees). | ||
{| border="1" cellpadding="20" cellspacing="0" | {| border="1" cellpadding="20" cellspacing="0" | ||
|- | |- | ||
|Time Start | |Time Start | ||
|Time Stop | |Time Stop | ||
− | |Time elapsed ( | + | |Time elapsed (hour) |
|Singles Count (on top) | |Singles Count (on top) | ||
|Coinc. Counts | |Coinc. Counts | ||
− | |Coinc. per | + | |Coinc. per hour |
|<math>\sqrt{N}</math> | |<math>\sqrt{N}</math> | ||
− | |<math>(x_i-\bar{x})^2</math> | + | |<math>\sqrt{(x_i-\bar{x})^2}</math> |
+ | |- | ||
+ | |1:20 pm || 2:20 pm ||1 ||5694 ||127 || 127 || 11.3 ||11 | ||
+ | |- | ||
+ | |2:20 pm || 3:20 pm ||1 ||4896 ||136 || 136 || 11.6 ||2 | ||
|- | |- | ||
− | | | + | |3:20 pm || 4:20 pm ||1 ||4655 ||151 || 151 || 12.2 ||13 |
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | |. | ||
− | | | ||
|}<br> | |}<br> | ||
+ | |||
+ | Mean <math>\mu</math> = 138 counts per hour | ||
+ | |||
+ | Instrumental Uncertainty =<math>\sigma = \sqrt{\frac{\sum (x_i - \bar{x})^2}{N-1}} = 12.12</math> counts per hour | ||
+ | |||
+ | The instrumental uncertainty is approximately equal to the Poisson sigma (<math>\sqrt{138}= 11.7</math>) counts per hour. | ||
+ | |||
+ | The cosmic ray telescope counting experiment appears to be following Poisson statistics. | ||
+ | [http://www.iac.isu.edu/mediawiki/index.php/Statistics_for_Experimenters See Statistics for Experimentalists] |
Latest revision as of 21:42, 19 September 2007
Angular Distribution | ||||||||
---|---|---|---|---|---|---|---|---|
Time Start | Time Stop | Time elapsed (min.; hour) | Thresholds on both Scintillators | Singles Count (on top) | Coinc. Counts | Coinc. per minute | Coinc. per Hour | Angle measure |
1:35 pm on 8/31 | 1:10 pm on 9/04 | 5725 min; 95.42 hr | 225 | 626816 | 1654 | .2889 | 17.33 | 75 degrees |
Cosmic rates measured each hour when the telecope accepts cosmics which intersect the earth's surface perpendicularly (defined as zero degrees).
Time Start | Time Stop | Time elapsed (hour) | Singles Count (on top) | Coinc. Counts | Coinc. per hour | ||
1:20 pm | 2:20 pm | 1 | 5694 | 127 | 127 | 11.3 | 11 |
2:20 pm | 3:20 pm | 1 | 4896 | 136 | 136 | 11.6 | 2 |
3:20 pm | 4:20 pm | 1 | 4655 | 151 | 151 | 12.2 | 13 |
Mean
= 138 counts per hourInstrumental Uncertainty =
counts per hourThe instrumental uncertainty is approximately equal to the Poisson sigma (
) counts per hour.The cosmic ray telescope counting experiment appears to be following Poisson statistics. See Statistics for Experimentalists