Difference between revisions of "Sample data table"
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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 || 2: pm || 1 || || || || || | + | |1: pm || 2: pm || 1 || || || || || || |
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| + | |2: pm || 3: pm || 1 || || || || || || | ||
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| − | | | + | |3:pm || 4: pm || 1 || || || || || || |
| − | |||
| − | |||
|- | |- | ||
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| − | | || || || || || || || <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 || || || || || | |1: pm || 4: pm || 3 || || || || || | ||
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| + | Cosmic rates measured when the telecope accepts cosmics which intersect the earth's surface at 30 degrees to the perpendicular. | ||
{| border="5" | {| border="5" | ||
| − | ! Date || Start Time || End Time || Singles Counts Top (N_1) || Singles Counts Bottom (N_2)|| <math>\frac{N_1-N_2}{N_1+N_2}</math> || Coincidence Counts || Coinc/Hour || Coinc/min || <math>\sqrt{N}</math> || <math>\sqrt{(x_i-\bar{x})^2}</math> || | + | ! Run Number || Date || Start Time || End Time || Run Time || Singles Counts Top (N_1) || Singles Counts Bottom (N_2)|| <math>\frac{N_1-N_2}{N_1+N_2}</math> || Coincidence Counts || Coinc/Hour || Coinc/min || <math>\sqrt{N}</math> |
| + | |- | ||
| + | | || 11/ to 11/ || 4: pm || 1: pm || 21 || || || || || || || | ||
| + | |}<br> | ||
| + | |||
| + | |||
| + | |||
| + | Cosmic rates measured each hour when the telecope accepts cosmics which intersect the earth's surface perpendicularly (defined as zero degrees). | ||
| + | {| border="5" | ||
| + | ! Run Number || Date || Start Time || End Time || Run Time || Singles Counts Top (N_1) || Singles Counts Bottom (N_2)|| <math>\frac{N_1-N_2}{N_1+N_2}</math> || Coincidence Counts || Coinc/Hour || Coinc/min || <math>\sqrt{N}</math> || <math>\sqrt{(x_i-\bar{x})^2}</math> | ||
| + | |- | ||
| + | | || 11/ || 1: pm || 2: pm || 1 || || || || || || || || | ||
| + | |- | ||
| + | | || 11/ || 2: pm || 3: pm || 1 || || || || || || || || | ||
| + | |- | ||
| + | | || 11/ || 3: pm || 4: pm || 1 || || || || || || || || | ||
| + | |- | ||
| + | | || || || || || || || || || || || ||<math>\sigma = \sqrt{\frac{\sum (x_i - \bar{x})^2}{N-1}}</math> | ||
|- | |- | ||
| − | ||||||||||||||||||||||||| | + | | || 11/ || 1: pm || 4: pm || 3 || || || || || || || || |
|}<br> | |}<br> | ||
Latest revision as of 21:00, 3 December 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 when the telecope accepts cosmics which intersect the earth's surface at 30 degrees to the perpendicular.
| Run Number | 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).
| Run Number | 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 |