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The Primary Aberrations  91

        curled inward. The wave front shown is “ahead” of the reference sphere;
        the distance by which it is ahead is called the optical path difference,
        or OPD, and is customarily expressed in units of wavelengths. The
        wave fronts associated with axial aberrations are symmetrical figures
        of rotation, in contrast to the off-axis aberrations such as coma and
        astigmatism. For example, the wave front for astigmatism would be a
        section of a torus (the outer surface of a doughnut) with different radii
        in the prime meridians. For off-axis imagery, the reference sphere is
        chosen to pass through the center of the exit pupil (in some calcula-
        tions, the reference sphere has an infinite radius, for convenience in
        computing).


        5.7  Aberration Correction and Residuals
        Section 5.4 indicated two methods which are used to control aberra-
        tions in simple optical systems, namely lens shape and stop position.
        For many applications a higher level of correction is needed, and it is
        then necessary to combine optical elements with aberrations of opposite
        signs so that the aberrations contributed to the system by one element
        are cancelled out, or corrected, by the others. A typical example is the
        achromatic doublet used for telescope objectives, shown in Fig. 5.18.
        A single positive element would be afflicted with both undercorrected
        spherical aberration and undercorrected chromatic aberration. In a
        negative element, in the other hand, both aberrations are overcorrected.
        In the doublet a positive element is combined with a less powerful
        negative element in such a way that the aberrations of each balance
        out. The positive lens is made of a (crown) glass with a low chromatic
        dispersion, and the negative element of a (flint) glass with a high
        dispersion. Thus, the negative element has a greater amount of chro-
        matic aberration per unit of power, by virtue of its greater dispersion,
        than the crown element. The relative powers of the elements are chosen
        so that the chromatic exactly cancels while the focusing power of the
        crown element dominates.
          The situation with regard to spherical aberration is quite analogous
        except that element power, shape, and index of refraction are involved
        instead of power and dispersion as in chromatic. If the index of the






                                            Figure 5.18 Achromatic doublet
                                            telescope objective. The powers
                                            and shapes of the two elements
                                            are so arranged that each cancels
                                            the aberrations of the other.
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