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Optical System Considerations  59

          Multiplying by yy p and rearranging, we get
                           y nu   ynu   y n′u′   yn′u′
                            p         p   p           p
        Note that on the left side of the equation the angles and indices are for
        the left side of the surface (that is, before refraction) and that on the
        right side of the equation the terms refer to the same quantities after
        refraction. Thus y p nu   ynu p is a constant which is invariant across
        any surface.
          By a similar series of operations based on Eq. 3.17, we can show that
        (y p nu   ynu p ) for a given surface is equal to (y p nu   ynu p ) for the next
        surface. Thus this term is not only invariant across the surface but also
        across the space between the surfaces; it is therefore invariant through-
        out the entire optical system or any continuous part of the system.

           Invariant     Inv   y nu   ynu   n (y u   yu )           (4.14)
                                p        p      p      p

        The invariant and magnification
        As an example of its application, we now write the invariant for the
        object plane and image plane of Fig. 4.4. In an object plane y p   h,
        n   n, y   0, and we get

                            Inv   hnu   (0) nu   hnu
                                              p
          In the corresponding image plane y p   h′, n   n′, y   0, and we get
                          Inv   h′n′u′  (0) n′u′   h′n′u′
                                              p
        Equating the two expressions gives

                                   hnu   h′n′u′                     (4.15)
        which can be rearranged to give a very generalized expression for the
        magnification of an optical system
                                       h′    nu
                                 m                                  (4.16)
                                       h    n′u′
          Equation 4.16 is, of course, valid only for the extended paraxial
        region; this relationship is sometimes applied to trigonometric calcu-
        lations, where it takes the form of Eq. 4.17 for the magnification at a
        zone of the aperture.
                               hn sin u   h′n′ sin u′               (4.17)
                                          n sin u
                                  or  m 5
                                         nrsin ur
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