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156   Chapter Four

















               FIGURE 4.31 Gray-scale display of the achromatized irradiance distribution.


               with Z o =−12 cm, and we choose a value d = 10.00 cm. Therefore,
                                                     o
                                                               √
               we select a focal distance for the achromatic lens f =  −Z o R o =
                                                                   2

               11.86 cm, and we place that object at a distance l = 2R o + f + f /d =
                                                                      o
               49.39 cm from that lens. A gray-scale display of the output irradiance
               is presented in Fig. 4.31. The comparison between this result and the
               monochromatic one in Fig. 4.30a shows the high achromatization level
               obtained with the optimized system.
               4.4.2 Controlling the Axial Response:
                      Synthesis of Pupil Masks by RWT
                      Inversion
               In Sec. 4.3.1.1 we showed that the axial behavior of the irradiance
               distribution provided by a system with an arbitrary value of SA can
               be obtained from the single RWT of the mapped pupil q 0,0 (s) of the
               system. In fact, Eq. (4.74) can be considered the keystone of a pupil
               design method 55  in which the synthesis procedure starts by perform-
               ing a tomographic reconstruction of W q (x,  ) from the projected
                                                  0,0
               function I (0, 0,z) representing the irradiance at the axial points—
               variable W 20 —for a sufficient set of values of W 40 . Thus, the entire
               two-dimensional Wigner space can be sampled on a set of lines de-
               fined by these parameters. The backprojection algorithm converts the
               desired axial irradiance for a fixed value of W 40 , represented by a one-
               dimensional function, to a two-dimensional function by smearing it
               uniformly along the original projection direction (see Fig. 4.8). Then
               the algorithm calculates the summation function that results when all
               backprojections are summed over all projection angles  , i.e., for all
               the different values of W 40 . The final reconstructed function W q (x,  )
                                                                   0,0
               is obtained by a proper filtering of the summation image. 55  Once the
               WDF is synthesized with the values of the input axial irradiances, the
               pupil function is obtained by use of Eq. (4.4). Finally, the geometric
               mapping in Eq. (4.57) is inverted to provide the desired pupil function.
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