TF ErrorAna PropOfErr: Difference between revisions
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http://www.physics.uoguelph.ca/~reception/2440/StatsErrorsJuly26-06.pdf | http://www.physics.uoguelph.ca/~reception/2440/StatsErrorsJuly26-06.pdf | ||
==Counting Experiment Example== | |||
The table below reports 8 measurements of the coincidence rate observed by two scintillators detecting cosmic rays. The scintillator are place a distance (x) away from each other in order to detect cosmic rays falling on the earth's surface. The time and observed coincidence counts are reported in separate columns as well as the angle made by the normal to the detector with the earths surface. Is the variation statistical? | |||
<math>\sigma^2_{Poisson} = \mu =</math> Mean Coinc/Hr | <math>\sigma^2_{Poisson} = \mu =</math> Mean Coinc/Hr | ||
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! Date || Time (hrs) || <math>\theta</math> ||Coincidence Counts || Mean Coinc/Hr || <math>\sqrt{Mean Counts/Hr}</math> || <math>\left | \sigma \right |</math> from Mean | ! Date || Time (hrs) || <math>\theta</math> ||Coincidence Counts || Mean Coinc/Hr || <math>\sqrt{Mean Counts/Hr}</math> || <math>\left | \sigma \right |</math> from Mean | ||
|- | |- | ||
|9/12/07 || 20.5 || | |9/12/07 || 20.5 || 30|| 2233 || 109 || 10.4 ||1 | ||
|- | |- | ||
|9/14/07 || 21 || | |9/14/07 || 21 || 30 || 1582 || 75 || 8.7||2 | ||
|- | |- | ||
|10/3/07 || 21 || | |10/3/07 || 21 || 30 || 2282 || 100 || 10.4||1 | ||
|- | |- | ||
|10/4/07 || 21 || | |10/4/07 || 21 || 30 || 2029 || 97 || 9.8|| 0.1 | ||
|- | |- | ||
|10/15/07 || 21 || | |10/15/07 || 21 || 30 || 2180 || 100 || 10|| 0.6 | ||
|- | |- | ||
|10/18/07 || 21 || | |10/18/07 || 21 || 30 || 2064 || 99 || 9.9||0.1 | ||
|- | |- | ||
| 10/23/07 || 21 || | | 10/23/07 || 21 || 30 || 2003 || 95 || 9.7||0.2 | ||
|- | |- | ||
| 10/26/07 || 21 || | | 10/26/07 || 21 || 30 || 1943 || 93 || 9.6 || 0.5 | ||
|} | |} | ||
Revision as of 23:38, 1 March 2010
Instrumental and Statistical Uncertainties
http://www.physics.uoguelph.ca/~reception/2440/StatsErrorsJuly26-06.pdf
Counting Experiment Example
The table below reports 8 measurements of the coincidence rate observed by two scintillators detecting cosmic rays. The scintillator are place a distance (x) away from each other in order to detect cosmic rays falling on the earth's surface. The time and observed coincidence counts are reported in separate columns as well as the angle made by the normal to the detector with the earths surface. Is the variation statistical?
[math]\displaystyle{ \sigma^2_{Poisson} = \mu = }[/math] Mean Coinc/Hr
| Date | Time (hrs) | [math]\displaystyle{ \theta }[/math] | Coincidence Counts | Mean Coinc/Hr | [math]\displaystyle{ \sqrt{Mean Counts/Hr} }[/math] | [math]\displaystyle{ \left | \sigma \right | }[/math] from Mean |
|---|---|---|---|---|---|---|
| 9/12/07 | 20.5 | 30 | 2233 | 109 | 10.4 | 1 |
| 9/14/07 | 21 | 30 | 1582 | 75 | 8.7 | 2 |
| 10/3/07 | 21 | 30 | 2282 | 100 | 10.4 | 1 |
| 10/4/07 | 21 | 30 | 2029 | 97 | 9.8 | 0.1 |
| 10/15/07 | 21 | 30 | 2180 | 100 | 10 | 0.6 |
| 10/18/07 | 21 | 30 | 2064 | 99 | 9.9 | 0.1 |
| 10/23/07 | 21 | 30 | 2003 | 95 | 9.7 | 0.2 |
| 10/26/07 | 21 | 30 | 1943 | 93 | 9.6 | 0.5 |
[math]\displaystyle{ \frac{\sum CPM_i}{8} = 97.44 }[/math]
[math]\displaystyle{ \frac{\sum Counts}{\sum time} = \frac{16316}{167.5}=97.41 }[/math]
The above 2 expressions are equivalent because all the denominators are essentially the value 21
[math]\displaystyle{ \frac{sum (x_i-\mu)^2}{8-1} = 10.8 }[/math]
P=68% = Probability that a measurement of a Gaussian variant will lie within 1 [math]\displaystyle{ \sigma }[/math] of the mean
- [math]\displaystyle{ = 0.68 * 8 = 5 }[/math]
Looks like we have 7/8 events within 1[math]\displaystyle{ \sigma }[/math] = 87.5%
Taylor Expansion
A quantity which is calculated using quantities with known uncertainties will have an uncertainty based upon the uncertainty of the quantities used in the calculation.
To determine the uncertainty in a quantity which is a function of other quantities, you can consider the dependence of these quantities in terms of a tayler expansion
Consider a calculation of a Table's Area
[math]\displaystyle{ A= L \times W }[/math]
The mean that the Area (A) is a function of the Length (L) and the Width (W) of the table.
[math]\displaystyle{ A = f(L,W) }[/math]
The Taylor series expansion of a function f(x) about the point a is given as
[math]\displaystyle{ f(x) = f(a) + \left . f^{\prime}(x)\right |_{x=a} \frac{x}{1!} + \left . f^{\prime \prime}(x)\right |_{x=a} \frac{x^2}{2!} + ... }[/math]
- [math]\displaystyle{ = \left . \sum_{n=0}^{\infty} f^{(n)}(x)\right |_{x=a} \frac{x^n}{n!} }[/math]
For small values of x (x << 1) we can expand the function about 0 such that
[math]\displaystyle{ \sqrt{1+x} = \left . \sqrt{1-0} \frac{1}{2}(1+x)^{-1/2}\right |_{x=0} \frac{x^1}{1!}+ \left . \frac{1}{2}\frac{-1}{2}(1+x)^{-3/2} \right |_{x=0} \frac{x^2}{2!} }[/math]
- [math]\displaystyle{ =1 + \frac{x}{2} - \frac{x^2}{4} }[/math]
The talylor expansion of a function with two variables[math]\displaystyle{ (x_1 , x_2) }[/math] about the average of the two variables[math]\displaystyle{ (\bar {x_1} , \bar{x_2} ) }[/math] is given by
[math]\displaystyle{ f(x_1, x_2)=f(\bar {x}_1, \bar{x}_2)+(x_1-\bar {x}_1) \frac{\partial f}{\partial x_1}\bigg |_{(x_1 = \bar {x}_1, x_2 = \bar{x}_2)} +(x_2-\bar{x}_2) \frac{\partial f}{\partial x_2}\bigg |_{(x_1 = \bar {x}_1, x_2 = \bar{x}_2)} }[/math]
or
[math]\displaystyle{ f(x_1, x_2)-f(\bar {x}_1, \bar{x}_2)=(x_1-\bar {x}_1) \frac{\partial f}{\partial x_1}\bigg |_{(x_1 = \bar {x}_1, x_2 = \bar{x}_2)} +(x_2-\bar{x}_2) \frac{\partial f}{\partial x_2}\bigg |_{(x_1 = \bar {x}_1, x_2 = \bar{x}_2)} }[/math]
The term
[math]\displaystyle{ f(x_1, x_2)-f(\bar {x}_1, \bar{x}_2) }[/math]
represents a small fluctuation of the function from its average [math]\displaystyle{ f(\bar {x}_1, \bar{x}_2) }[/math] if we ignore higher order terms in the Taylor expansion ( this means the fluctuations are small).
Based on the Definition of Variance
- [math]\displaystyle{ \sigma^2 = \frac{\sum_{i=1}^{i=N} (x_i - \bar{x})^2}{N} }[/math]
We can write the variance of the area
- [math]\displaystyle{ \sigma^2_A = \frac{\sum_{i=1}^{i=N} (A_i - \bar{A})^2}{N} }[/math]
- [math]\displaystyle{ = \frac{\sum_{i=1}^{i=N} \left [ (L-\bar{L}) \frac{\partial A}{\partial L} \bigg |_{\bar L \bar W} + (W-\bar W) \frac{\partial A}{\partial W} \bigg |_{\bar L \bar WW} \right] ^2}{N} }[/math]
- [math]\displaystyle{ = \frac{\sum_{i=1}^{i=N} \left [ (L-\bar{L}) \frac{\partial A}{\partial L} \bigg |_{\bar L \bar W} \right ] ^2}{N} + \frac{\sum_{i=1}^{i=N} \left [ (W-\bar W) \frac{\partial A}{\partial W} \bigg |_{\bar L \bar W} \right] ^2 }{N} }[/math]
- [math]\displaystyle{ +2 \frac{\sum_{i=1}^{i=N} \left [ (L-\bar{L}) (W-\bar W) \frac{\partial A}{\partial L} \bigg |_{\bar L \bar W} \frac{\partial A}{\partial W} \bigg |_{\bar L \bar W} \right]^2}{N} }[/math]
- [math]\displaystyle{ = \sigma^2_L \left ( \frac{\partial A}{\partial L} \right )^2 +\sigma^2_W \left ( \frac{\partial A}{\partial W} \right )^2 + 2 \sigma^2_{LW} \frac{\partial A}{\partial L} \frac{\partial A}{\partial W} }[/math]
where [math]\displaystyle{ \sigma^2_{LW} = \frac{\sum_{i=1}^{i=N} \left [ (L-\bar{L}) (W-\bar W) \right ]^2}{N} }[/math] is defined as the Covariance between [math]\displaystyle{ L }[/math] and [math]\displaystyle{ W }[/math].
Weighted Mean and variance
If each observable ([math]\displaystyle{ x_i }[/math]) is accompanied by an estimate of the uncertainty in that observable ([math]\displaystyle{ \delta x_i }[/math]) then weighted mean is defined as
- [math]\displaystyle{ \bar{x} = \frac{ \sum_{i=1}^{i=n} \frac{x_i}{\delta x_i}}{\sum_{i=1}^{i=n} \frac{1}{\delta x_i}} }[/math]
The variance of the distribution is defined as
- [math]\displaystyle{ \bar{x} = \sum_{i=1}^{i=n} \frac{1}{\delta x_i} }[/math]
| Date | Time (hrs) | [math]\displaystyle{ \theta }[/math] | Coincidence Counts | Coinc/Hour | [math]\displaystyle{ \sqrt{N} }[/math] |
|---|---|---|---|---|---|
| 9/6/07 | 18 | 45 | 1065 | 59.2 | |
| 9/7/07 | 14.66 | 45 | 881 | 60.1 | |
| 9/9/07 | 43 | 60 | 1558 | 36.23 | |
| 9/12/07 | 20.5 | 330 | 2233 | 108.93 | |
| 9/13/07 | 21 | 315 | 2261 | 107.67 | |
| 9/14/07 | 21 | 330 | 1582 | 75.33 | |
| 9/18/07 | 21 | 300 | 1108 | 52.8 | |
| 9/19/07 | 21 | 300 | 1210 | 57.62 | |
| 9/20/07 | 21 | 300 | 1111 | 52.69 | |
| 9/21/07 | 21 | 300 | 1012 | 57.62 | |
| 9/26/07 | 21 | 315 | 1669 | 79.48 | |
| 9/27/07 | 21 | 315 | 1756 | 83.29 | |
| 9/29/07 | 24.5 | 315 | 2334 | 95.27 | |
| 10/3/07 | 21 | 330 | 2282 | 108.67 | |
| 10/4/07 | 21 | 330 | 2029 | 96.62 | |
| 10/10/07 | 21 | 315 | 1947 | 92.71 | |
| 10/15/07 | 69 | 330 | 2180 | 31.59 | |
| 10/18/07 | 21 | 330 | 2064 | 98.52 | |
| 10/23/07 | 21 | 330 | 2003 | 95.38 | |
| 10/26/07 | 21 | 330 | 1943 | 92.52 | |
| 11/2/07 | 21 | 330 | 2784 | ||
| 11/5/07 | 69 | 330 | 10251 | 148.57 | |
| 11/16/07 | 21 | 30 | 3581 | 170.52 |