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Principles of Radiometry and Photometry  257

        with a radiance of N W ster  1  cm  2  and an intensity of J     J 0 cos
        NA cos   W/ster. The incremental ring area on a hemisphere of radius R
        has an area of 2 R sin    R d  and thus subtends (from A) a solid angle
              2
                         2
        of 2 R sin   d /R   2  sin   d  steradians. The radiation intercepted
        by this ring is the product of the intensity of the source and the solid
        angle, or
                     dP   J 2  sin   d    2 NA sin   cos   d        (12.3)

        Integrating to find the total power radiated into the hemisphere from
        A, we get

                                               2
               /2                           sin     /2
        P   
 2 NA sin   cos   d    2 NA               NA watts     (12.4)
             0                                2    0
        Dividing by A to get watts emitted per square centimeter of source,
        we find the radiation into the 2  steradian of the hemisphere to be
         N W/cm , not 2 N. This is the basic relationship between radiance and
                 2
        the power emitted from the surface.


        12.5 Irradiance Produced by a Diffuse
        Source
        It is frequently of interest to determine the irradiance produced at a
        point by a lambertian source of finite size. Referring to Fig. 12.3,
        assume that the source is a circular disk of radius R and that we wish
        to determine the irradiance at some point X which is a distance S from
        the source and is on the normal through the center of the source. (Note
        that we will determine the irradiance on a plane parallel to the plane
        of the source.) The radiant intensity of a small element of area dA in
        the direction of point X is given by Eq. 12.2 as

                             J   J cos    N dA cos
                                  0












                                          Figure 12.3 Geometry of a circu-
                                          lar source irradiating point X.
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