Difference between revisions of "September 4, 2007 - Cosmic Telescope"
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− | ! colspan="2"| | + | ! colspan="2"|Angular Distribution |
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|Time Start | |Time Start |
Revision as of 20:04, 12 September 2007
Angular Distribution | ||||||||
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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 | 121 |
2:20 pm | 3:20 pm | 1 | 4896 | 136 | 136 | 11.6 | 4 |
3:20 pm | 4:20 pm | 1 | 4655 | 151 | 151 | 12.2 | 169 |
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