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Date: 11-3-2021
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Date: 1-4-2021
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The probability that a random sample from an infinite normally distributed universe will have a mean within a distance of the mean of the universe is
(1) |
where is the normal distribution function and is the observed value of
(2) |
The probable error is then defined as the value of such that , i.e.,
(3) |
which is given by
(4) |
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(5) |
(OEIS A092678; Kenney and Keeping 1962, p. 134). Here, is the inverse erf function. The probability of a deviation from the true population value at least as great as the probable error is therefore 1/2.
REFERENCES:
Kenney, J. F. and Keeping, E. S. Mathematics of Statistics, Pt. 1, 3rd ed. Princeton, NJ: Van Nostrand, pp. 129 and 134, 1962.
Sloane, N. J. A. Sequence A092678 in "The On-Line Encyclopedia of Integer Sequences."
Whittaker, E. T. and Robinson, G. The Calculus of Observations: A Treatise on Numerical Mathematics, 4th ed. New York: Dover, p. 184, 1967.
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