Cf_f_(i,j)=Cf_f_(ij),(7.83)

in other words, we require statistical invariance under translations, which is actually quite a strong restriction on the object. The imaging process is again modeled as

X_=(P_*f_)+ξ_,(7.84)

with the PSF P_and independent Gaussian noise ξ with variance σ2. The idea underlying the Wiener filter is to recover the original object f by convolution of the image X with a function h. To this end, h has to be chosen such that the average discrepancy between hX and f is minimal

E[ (h_*X_f)2 ]=E[ Z_2 ]2E[ Z_f_ ]+E[ f_2 ]=i(CZ_Z_(i,i)2CZ_f_(i,i)+Cf_f_(i,i)),(7.85)

where single components Zi of Z are

Zi=jhjXij.(7.86)

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