Difference between revisions of "October 4, 2007 - Cosmic Telescope"
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|<math>\sqrt{(x_i-\bar{x})^2}</math> | |<math>\sqrt{(x_i-\bar{x})^2}</math> | ||
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− | | | + | |4:01 pm of 10/3 || 1:01 pm of 10/3 || 21 || 142005 || 2282 || 108.67 || 2.27 || |
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|<math>\sqrt{(x_i-\bar{x})^2}</math> | |<math>\sqrt{(x_i-\bar{x})^2}</math> | ||
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− | |1: pm || | + | |1:02 pm || 1:32 pm || .5 || 2697 || 57 || 114 || 15.1 || |
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− | |2: pm || 3: pm || | + | |2:25 pm || 3:25 pm || 1 || 5000 || 135 || 135 || 11.62 || |
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− | |3: pm || | + | |3:25 pm || 3:55 pm || .5 || 66 || 132 || 132 || 11.49 || |
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Revision as of 21:27, 12 October 2007
Cosmic rates measured each hour when the telecope accepts cosmics which intersect the earth's surface at 315 degrees to the perpendicular.
Time Start | Time Stop | Time elapsed (hour) | Singles Count (on top) | Coinc. Counts | Coinc. per hour | ||
4:01 pm of 10/3 | 1:01 pm of 10/3 | 21 | 142005 | 2282 | 108.67 | 2.27 |
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 | ||
1:02 pm | 1:32 pm | .5 | 2697 | 57 | 114 | 15.1 | |
2:25 pm | 3:25 pm | 1 | 5000 | 135 | 135 | 11.62 | |
3:25 pm | 3:55 pm | .5 | 66 | 132 | 132 | 11.49 | |
1: pm | 4: pm |