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220   Chapter Seven


               Total radiant power in terms of L is given by

                                (z) =     L( r, ˆ n) cos   d	 dA     (7.7)
                                     A 1/2
               In this expression, the z value indicates the source location on the z
               axis. The symbol A under the integral stands for the integration over
               the area of the source, and the 1/2 under the integral implies the
               angle integration is limited to the right half space, 0 ≤   ≤  /2 and
               0 ≤ 	 ≤ 2 . The product cos   d	 is called the projected solid angle
               differential element. Following Eq. (7.7), the spectral radiant power
                                                       ˆ
                ˆ
                (z,  ) is found by using the spectral radiance L( r, ˆ n,  ) with units of
                            −1
                    −2
                        −1
               Wcm sr Hz .
                 Far enough away from the source, the details of the source struc-
               ture become less important but the characteristic angular distribu-
               tion of radiation assumes importance. To describe this situation, the
               term radiant intensity I (z, ˆ n) with units W sr −1  is used. Its solid angle
               integral over the right half-space yields the total radiant power

                                     (z) =   I (z, ˆ n) d	           (7.8)
                                          1/2
                                                              ˆ
               The solid angle integral over the spectral radiant intensity I(z, ˆ n,  ) with
                          −1
               units of W sr Hz −1  yields the total spectral radiant power.
                 Among the various functions defined above, the basic one is the
                               ˆ
               spectral radiance L( r, ˆ n,  ). In terms of it, the other functions may
               be derived by regrouping and performing the appropriate integral.
               The interrelationships among the spectral functions are displayed in
               Table 7.1.


                                 ˆ
                                L( r, ˆ n,  ), [W cm −2 sr −1 Hz −1 ]

                              ˆ           ˆ
                               (z,  ) =   L( r, ˆ n,  ) cos   d	 dA
                                     A 1/2

                  ˆ         ˆ                 ˆ              ˆ
                  M( r,  ) =  L( r, ˆ n,  ) cos   d	  I(z, ˆ n,  ) = cos    L( r, ˆ n,  ) dA
                         1/2                               A

                     ˆ         ˆ                 ˆ         ˆ
                     (z,  ) =  M( r,  ) dA       (z,  ) =  I(z, ˆ n,  ) d
                            A                           1/2

               TABLE 7.1 Interrelationships among the Spectral Functions of
               Conventional Radiometry
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