Difference between revisions of "November 8, 2007 - Cosmic Telescope"

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Cosmic rates measured each hour when the telecope accepts cosmics which intersect the earth's surface at 330 degrees to the perpendicular.
 
Cosmic rates measured each hour when the telecope accepts cosmics which intersect the earth's surface at 330 degrees to the perpendicular.
{| border="1" cellpadding="20" cellspacing="0"
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{| border="5"
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! 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>
 
|-
 
|-
|Time Start
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|4: pm of 11/ || 1: pm of 11/ || 21 ||  ||  ||  || || || ||
|Time Stop
 
|Time elapsed (hour)
 
|Singles Counts (on top)
 
|Singles Counts (on bottom)
 
|Coinc. Counts
 
|Coinc. per hour
 
|<math>\sqrt{N}</math>
 
|<math>\sqrt{(x_i-\bar{x})^2}</math>
 
|-
 
|4: pm of 11/ || 1: pm of 11/ || 21 ||  ||  ||  || || ||  
 
 
|}<br>
 
|}<br>
  
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Cosmic rates measured each hour when the telecope accepts cosmics which intersect the earth's surface perpendicularly (defined as zero degrees).
 
Cosmic rates measured each hour when the telecope accepts cosmics which intersect the earth's surface perpendicularly (defined as zero degrees).
{| border="1" cellpadding="20" cellspacing="0"
+
{| 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>  
|Time Start
 
|Time Stop
 
|Time elapsed (hour)
 
|Singles Count (on top)
 
|Singles Counts (on bottom)
 
|Coinc. Counts
 
|Coinc. per hour
 
|<math>\sqrt{N}</math>
 
|<math>\sqrt{(x_i-\bar{x})^2}</math>
 
|-
 
|1: pm || 2: pm || 1 ||  ||  ||  ||  ||
 
 
|-
 
|-
|2: pm || 3: pm || 1 ||  ||  ||  ||  ||  
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|1: pm || 2: pm || 1 ||  ||  ||  ||  || || || ||
 
|-
 
|-
|3:pm || 4: pm || 1 ||  ||  ||  ||  ||  
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|2: pm || 3: pm || 1 ||  ||  ||  ||  || || || ||
 
|-
 
|-
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|3:pm || 4: pm || 1 ||  ||  ||  ||  || || || ||
 
|-
 
|-
| || || || || || || || <math>\sigma = \sqrt{\frac{\sum (x_i - \bar{x})^2}{N-1}}</math>
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| || || || || || || || || || ||<math>\sigma = \sqrt{\frac{\sum (x_i - \bar{x})^2}{N-1}}</math>
 
|-
 
|-
|1: pm || 4: pm || 3 ||  ||  ||  ||  ||  
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|1: pm || 4: pm || 3 ||  ||  ||  ||  || || || ||
 
|}<br>
 
|}<br>

Latest revision as of 22:29, 4 December 2007

128


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 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]
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).

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]
1: pm 2: pm 1
2: pm 3: pm 1
3:pm 4: pm 1
[math]\sigma = \sqrt{\frac{\sum (x_i - \bar{x})^2}{N-1}}[/math]
1: pm 4: pm 3