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116   Chapter Six

        The relations between the thin-lens contributions and the various
        measures of the aberrations are the same as indicated in Sec. 6.3.
                      2
                     n (n   1)                 2 (n   1) (n   1)
               G                         G
                 1
                                           5
                         2                            n
                     (2n   1) (n   1)          (3n   2) (n   1)
                G                        G
                 2
                                           6
                            2                        2n
                                                                   (6.3u)
                     (3n   1) (n   1)          (2n   1) (n   1)
                G                        G
                 3
                                           7
                            2                        2n
                      (n   2) (n   1)          n (n   1)
                G                        G
                 4
                                           8
                           2n                      2
                                     ∗
                                ∗
          The contributions, TSC , CC , etc., are determined for each element
        in the system. The individual contributions are then added to get
              ∗
                    ∗
         TSC ,  CC , etc., and, to the extent that (1) the thin-lens fiction is
        valid, and (2) the third-order aberrations adequately represent the
        total aberration of the system,
                            SC ≈ L′   l′
                              ∗             1
                          CC ≈ coma S      ≈ 
 coma T
                                             3
                     ∗        ∗
                  PC   AC ≈ x s        (sagittal field curvature)
                    ∗         ∗
                 PC   3 AC ≈ x t       (tangential field curvature)
                            1
                                    Petzval radius


                             n
                     100  DC ∗
                               ≈ percentage distortion
                         h
                         LchC   l′ F    l′ C
                              ∗
                        TchC   h F     h C

                         SchC   l′ d    l′ C
          The thin-lens third-order aberration expressions (which are frequently
        called G-sums) can be used with the specific data of an optical system
        to determine the (approximate) aberration values. Another usage is in
        design work where the curvatures and/or spacings and powers of the
        elements are to be determined in such a way that the aberration
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