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Stops, Apertures, Pupils and Diffraction  195

























        Figure 9.17 (Upper) Prism spectrometer. (Lower) Grating
        spectrometer.



        it is also diffracted. As with the slit aperture discussed above, at certain
        angles the diffracted wavelets reinforce, and maxima are produced when
                                        m
                                sin          sin I                  (9.20)
                                         S
        where 	 is the wavelength, I is the angle of incidence, S is the spacing
        of the grating lines, m is an integer, called the order of the maxima,
        and the positive sign is used for a transmission grating, the negative
        for a reflecting. (Note that a sinusoidal grating has only a first order.)
        Since   depends on the wavelength 	, such a device can be used to sep-
        arate the diffracted light into its component wavelengths. When used
        as indicated in Fig. 9.17, the resolution of a grating is given by


                                          mN                        (9.21)
                                    d
        where m is the order and N is the total number of lines in the grating
        (assuming the size of the grating to be the limiting aperture of the
        system).


        9.11  Diffraction of a Gaussian (Laser) Beam
        The illumination distribution in the image of a point as described in
        Secs. 9.9 and 9.10 was based on the assumptions that the optical
        system was perfect and that both the transmission and the wave-front
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