Difference between revisions of "Sample data table"
Jump to navigation
Jump to search
Line 65: | Line 65: | ||
| || || || || || || || || || || ||<math>\sigma = \sqrt{\frac{\sum (x_i - \bar{x})^2}{N-1}}</math> | | || || || || || || || || || || ||<math>\sigma = \sqrt{\frac{\sum (x_i - \bar{x})^2}{N-1}}</math> | ||
|- | |- | ||
− | | || 1: pm || 4: pm || 3 | + | | 11/ || 1: pm || 4: pm || 3 || || || || || || || || |
|}<br> | |}<br> |
Revision as of 22:39, 27 November 2007
Cosmic rates measured each hour when the telecope accepts cosmics which intersect the earth's surface at 330 degrees to the perpendicular.
Time Start | Time Stop | Time elapsed (hour) | Singles Counts (on top) | Singles Counts (on bottom) | Coinc. Counts | Coinc. per hour | ||
4: pm of 11/ | 1: pm of 11/ | 21 |
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) | Singles Counts (on bottom) | Coinc. Counts | Coinc. per hour | ||
1: pm | 2: pm | 1 | ||||||
2: pm | 3: pm | 1 | ||||||
3:pm | 4: pm | 1 | ||||||
1: pm | 4: pm | 3 |
Cosmic rates measured each hour when the telecope accepts cosmics which intersect the earth's surface at 330 degrees to the perpendicular.
Date | Start Time | End Time | Run Time | Singles Counts Top (N_1) | Singles Counts Bottom (N_2) | Coincidence Counts | Coinc/Hour | Coinc/min | ||
---|---|---|---|---|---|---|---|---|---|---|
11/ to 11/ | 4: PM | 1: PM | 21 |
Cosmic rates measured each hour when the telecope accepts cosmics which intersect the earth's surface perpendicularly (defined as zero degrees).
Date | Start Time | End Time | Run Time | Singles Counts Top (N_1) | Singles Counts Bottom (N_2) | Coincidence Counts | Coinc/Hour | Coinc/min | |||
---|---|---|---|---|---|---|---|---|---|---|---|
11/ | 1: pm | 2: pm | 1 | ||||||||
11/ | 2: pm | 3: pm | 1 | ||||||||
11/ | 3:pm | 4: pm | 1 | ||||||||
11/ | 1: pm | 4: pm | 3 |