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Chapter
                                                                 6








                Third-Order Aberration Theory

                                           and Calculation















        6.1  Introduction
        The previous chapter described the various aberrations and, in Eqs. 5.1
        and 5.2, indicated the manner in which the various “orders” of aberra-
        tions varied with the aperture and the field angle of the optical system.
        For an axially symmetrical optical system only “odd” orders (1st, 3rd,
        5th, 7th . . .) may exist. The aberrations of the first-order turn out to be
        those which are eliminated by locating the reference point at the
        paraxial image. The first-order aberrations are thus defects of focus or
        of image size (or height) which vary linearly with aperture or obliquity,
        such as simple defocusing or the paraxial chromatic aberrations (e.g.,
        transverse axial chromatic or lateral color).
          And so we come to the first “real” aberrations, the third-order
        aberrations wherein the exponents of y (the aperture) and h (the field
        angle) add up to three. And then we find the fifth-order aberrations,
        followed by the seventh-, the ninth-, and so on. Limiting our attention
        to the third- and fifth-order, we have the five third-order aberrations,
        the five corresponding fifth-order aberrations, plus two new fifth-order
        aberrations, oblique spherical and elliptical coma. The manner in
        which the aberrations vary with aperture and field are tabulated on
        the next page:







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