|
Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node342.html
Дата изменения: Fri Feb 23 14:02:34 1996 Дата индексирования: Tue Oct 2 18:52:16 2012 Кодировка: Поисковые слова: redshift survey |
Let us consider a measured wavelet coefficient
at the scale i.
We assume
that its value, at a given scale and a given position,
results from a noisy process, with a Gaussian distribution with a
mathematical expectation
, and a standard deviation
:

Now, we assume that the set of expected coefficients
for a given
scale also follows a Gaussian distribution, with a null mean and a
standard deviation
:

The null mean value results from the wavelet property:

We want to get an estimate of
knowing
. Bayes' theorem gives:
We get:

where:

the probability
follows a Gaussian distribution with a mean:

and a variance:

The mathematical expectation of
is
.
With a simple multiplication of the coefficients by the constant
,
we get a linear filter. The algorithm is:
.
of the first plane
from the histogram of
. As we process oversampled images, the
values of the wavelet image corresponding to the first scale (
)
are due mainly to the noise. The histogram shows a Gaussian peak
around 0. We compute the standard deviation of this Gaussian
function, with a
clipping, rejecting pixels where the signal
could be significant;
from
. This
is done from the study of the variation of the noise between two
scales, with an hypothesis of a white gaussian noise;
where
is the variance of
.
.
.
.