Difference between revisions of "October 10, 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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− | |1:07 pm || 2:07 pm || 1 || 7169 || 137 || 137 || 11.70 || | + | |1:07 pm || 2:07 pm || 1 || 7169 || 137 || 137 || 11.70 || 2.67 |
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− | |2:07 pm || 4:07 pm || 2 || 20463 || 282 || 141 || 8.40 || | + | |2:07 pm || 4:07 pm || 2 || 20463 || 282 || 141 || 8.40 || 1.33 |
|- | |- | ||
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|- | |- | ||
− | |1:07 pm || 4:07 pm || 3 || 20463 || 419 || | + | |1:07 pm || 4:07 pm || 3 || 20463 || 419 || 139.67 || 1.68 || |
|}<br> | |}<br> |
Revision as of 20:33, 15 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 | ||
4:06 pm of 10/9 | 1:06 pm of 10/10 | 21 | 161038 | 1947 | 92.71 | 2.10 |
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 | ||
1:07 pm | 2:07 pm | 1 | 7169 | 137 | 137 | 11.70 | 2.67 |
2:07 pm | 4:07 pm | 2 | 20463 | 282 | 141 | 8.40 | 1.33 |
1:07 pm | 4:07 pm | 3 | 20463 | 419 | 139.67 | 1.68 |