Statistics for Experimenters: Difference between revisions
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= Definitions= | |||
;Accuracy | |||
: A measure of how close the experimental result is to the "true" value | |||
; Precisison | |||
: A meauser of close the result is determined without knowing the true vaule | |||
: Precision is often used to predict the accuracy of a quantity to be measured (you don't know the answer before doing the experiment) | |||
;Random Error | |||
: The error in a result due to the finite precision of an experiment | |||
: A measure of the statistical fluctuations which result after repeated experimentation | |||
;Systematic Error | |||
; Reproducable inaccuracies introduced by faulty equipment, calibration, or technique. | |||
=Probability Distributions= | |||
;Binomial distribtuion | ;Binomial distribtuion | ||
Revision as of 16:22, 5 September 2007
Definitions
- Accuracy
- A measure of how close the experimental result is to the "true" value
- Precisison
- A meauser of close the result is determined without knowing the true vaule
- Precision is often used to predict the accuracy of a quantity to be measured (you don't know the answer before doing the experiment)
- Random Error
- The error in a result due to the finite precision of an experiment
- A measure of the statistical fluctuations which result after repeated experimentation
- Systematic Error
- Reproducable inaccuracies introduced by faulty equipment, calibration, or technique.
Probability Distributions
- Binomial distribtuion
- best example is a coin toss, its either heads or tails
- mean ([math]\displaystyle{ \mu }[/math]) = number of tries [math]\displaystyle{ n }[/math](coin flips) * probability of success[math]\displaystyle{ p }[/math] (head, 1/2)
- standard deviation([math]\displaystyle{ \sigma }[/math]) = [math]\displaystyle{ np(1-p) }[/math]
- Poisson Distribution
- standard deviation ([math]\displaystyle{ \sigma }[/math]) = root of the mean ([math]\displaystyle{ \sqrt{\mu} }[/math])
- use in counting experiments
- the distribtuion approximates the Binomial Distribution for the special case when the mean ([math]\displaystyle{ \mu }[/math]) is a lot less than the number of attempts to measure ([math]\displaystyle{ n }[/math]) because the probability of the event occurrring is small.
- In the cosmic ray telescope experiment the mean number of detected cosmic rays is much smaller than the number of cosmic rays passing by.
- Gaussian/Normal Distribution
- Full WIdth at Half Max (FWHM) = width of the distribution at half the value of the maximum probabilty (distibution peak) = [math]\displaystyle{ \Gamma }[/math]
- standard deviation ([math]\displaystyle{ \sigma }[/math]) = [math]\displaystyle{ \frac{\Gamma} {2.354} }[/math]
- error = [math]\displaystyle{ 0.675 \sigma }[/math]