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Chapter
                                                                 7








                        Prism and Mirror Systems















        7.1  Introduction
        In most optical systems, prisms serve one of two major functions. In
        spectral instruments (spectroscopes, spectrographs, spectrophotometers,
        etc.) their function is to disperse the light or radiation; that is, to sepa-
        rate the different wavelengths. In other applications, prisms are used
        to displace, deviate, or reorient a beam of light or an image. In this type
        of use, the prism is carefully arranged so that it will not separate the
        different colors.


        7.2  Dispersing Prisms
        In a typical dispersing prism, as shown in Fig. 7.1, a light ray strikes
        the first surface at an angle of incidence I 1 and is refracted downward,
        making an angle of refraction I′ 1 with the normal to the surface. The
        ray is thus deviated through an angle of (I 1   I′ 1 ) at this surface. At
        the second surface the ray is deviated through an angle (I′ 2   I 2 ), so
        the total deviation of the ray is given by
                             D   (I   I′ )   (I′   I )               (7.1)
                                   1    1     2    2
          From the geometry of the figure it can be seen that angle I 2 is equal
        to (A   I′ 1 ), where A is the vertex angle of the prism; making this sub-
        stitution in Eq. 7.1, we get

                                 D   I   I′   A                      (7.2)
                                      1    2



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