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Anscombe transform : ウィキペディア英語版
Anscombe transform

In statistics, the Anscombe transform, named after Francis Anscombe, is a variance-stabilizing transformation that transforms a random variable with a Poisson distribution into one with an approximately standard Gaussian distribution. The Anscombe transform is widely used in photon-limited imaging (astronomy, X-ray) where images naturally follow the Poisson law. The Anscombe transform is usually used to pre-process the data in order to make the standard deviation approximately constant. Then denoising algorithms designed for the framework of additive white Gaussian noise are used; the final estimate is then obtained by applying an inverse Anscombe transformation to the denoised data.
==Definition==
For the Poisson distribution the mean m and variance v are not independent: m = v. The Anscombe transform〔

: A:x \mapsto 2\sqrt} \,
aims at transforming the data so that the variance is set approximately 1 whatever the mean. It transforms Poissonian data x (with mean m) to approximately Gaussian data of mean 2\sqrt - 1/(4\sqrt) and standard deviation 1. This approximation is valid provided that m is larger than 4.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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