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166   Chapter Eight

        sensitive to yellow-green light at a wavelength of 0.55   m, and its
        sensitivity drops off on either side of this peak. For most purposes the
        sensitivity of the eye may be considered to extend from 0.4 to 0.7  m.
        (or 0.38 to 0.78) Thus, in designing an optical instrument for visual
        use, the monochromatic aberrations are corrected for a wavelength of
        0.55 or 0.59  m and chromatic aberration is corrected by bringing the
        red and blue wavelengths to a common focus. The wavelengths usually
        chosen are either  e(0.5461   m) or  d(0.5876   m) for the yellow,
        C(0.6563  m) for the red, and F(0.4861  m) for the blue.
          Figure 8.8 shows the sensitivity of the eye as a function of wave-
        length for normal levels of illumination and also for the dark-adapted
                                                                      2
        eye. The photopic curve applies for brightness levels of 3 cd/m or
        more, and the scotopic curve applies for brightness levels of 0.003 cd/m 2
        or less. Between these levels, the term “mesopic” is used. Notice that
        the peak sensitivity for the dark-adapted eye shifts toward the blue
        end of the spectrum, from 0.55   m to a value near 0.51   m. This
        “Purkinje shift” is due to the differing chromatic sensitivities of the
        rods and cones of the retina, as shown in Fig. 8.8. Figure 8.9 is a tab-
        ulation of the values used in plotting Fig. 8.8.
          The sensitivity of the eye has been measured in the infrared out to
        1100 nm, where it is less than 10 –11  of the sensitivity at the peak
        response (at 555 nm). Figure 8.10 is a plot of both the photopic and
        scotopic spectral sensitivity which also has the integral of both plots,
        showing the fraction of the total response due to wavelengths shorter
        than the indicated one. This curve allows one to determine the rela-
        tive response between two wavelengths or to determine a suitable
        weighting for the wavelengths used in the analysis of an optival system’s
        performance.
          The Troland is a unit of retinal illumination and equals:

                                                2
                                                                   2
             Troland   (Object luminance in cd/m )/(Pupil area in mm )
                       278   (illuminance in lm/m 2 )







                                         Figure 8.8 The relative sensitiv-
                                         ity of the eye to different wave-
                                         lengths for normal levels of
                                         illumination (photopic vision)
                                         and under conditions of dark
                                         adaptation (scotopic vision).
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