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Imaging Systems: Phase-Space Representations      171


               We note that several interesting features are apparent from Eq. (5.11).
               First, independently of the value of x, the rays coming from the edge of
               the pupil (marginal rays) can be considered as having zero amplitude,
               W q (x, 	) = 0. Second, in a lax manner, one can consider that all the
               rayscomingtotheopticalaxis(x = 0)addconstructively.However,the
               amplitude of the rays decreases as 4(	 −| |). Third, in a lax manner,
               one can consider that outside the optical axis some of the rays add
               destructively. Specifically, at the point x = 1/2	, the amplitude of the
               rays varies as (2	/ ) sin[2 (1 −| /	|)].
                 According to Ref. 11, under the influence of wave aberrations, the
               WDF of the diffraction-limited system W 0 (x,  ) changes as follows:

                                 [M/2]       2m+1
                                 ,          ∂                  d
                  W(x,  ) = exp −    C m ( )  2m+1   W 0 x − f     ,
                                            ∂x                 d
                                 m=1
                                                                    (5.12)
               In Eq. (5.12) we employ the letter f for denoting the focal length of
               the optical processor;  ( ) denotes the wave aberration polynomial;
               [M/2] = M/2 − 1if M is an even integer number; and [M/2] =
               (M− 1)/2if M is an odd integer number. In the differential opera-
               tor, the coefficients are

                                           f  2m+1  d 2m+1
                                                                    (5.13)
                              C m ( ) =      2m       2m+1
                                       4            d
                                            (2m + 1)!
               It is apparent from Eq. (5.12) that the WDF W 0 (x,  ) suffers from lateral
               displacements, which are predicted by geometrical optics. In addition,
               the WDF modifies its amplitude distribution, as predicted by wave
               optics. 11
                 Next we discuss the use of an equivalent optical processor, as de-
               picted in Fig. 5.5, for implementing filtering operations in the phase-
               space representation. To that end, we represent the equivalent optical
               image processor, by the superposition integral
                                  ∞
                                ∞
                     W (x,  ) =     W 0 (x 0 ,   0 )W b (x,  ; x 0 ,   0 ) dx 0 d  0  (5.14)
                              −∞ −∞
               The impulse response W b (x,  ; x 0 ,   0 ) is the Bastiaans 12  double WDF.
               By simple comparison between Eqs. (5.9) and (5.14), one finds that for
               a space-invariant imaging system
                           W b (x,  ; x 0 ,   0 ) = W q (x − x 0 ,   0 ) (  −   0 )  (5.15)

                 Next, at the pupil aperture of the equivalent optical processor,
               we note that the complex amplitude distribution is the AF A 0 ( ,y).
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