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232   Chapter Seven


                 The total spectral radiant power is found to be
                                       =  AS BB ( ,T)               (7.49)

               The constant A is the area of the elementary hole in the blackbody
               cavity to provide the radiation to escape. The spectral radiant exitance
               evaluates to
                                  M(  s , 0,  ) =  S BB ( ,T)       (7.50)
                                     r
               Finally, the spectral radiant intensity can be shown to be

                                  J ( ˆ n,  ) = cos  AS BB ( ,T)    (7.51)
               We observe from Eqs. (7.48) to (7.51) that blackbody radiation is Lam-
               bertian; see Eq. (7.10).


               7.7.2 Non-coherent Source
               The spatial coherence function for a noncoherent 3, 5  source is defined
               by
                                              	    2
                             1        1
                                                    ˆ
                         r s +  r s12 ,  r s −  r s12 , 0,    =  I 0 ( )  ( r s12 )  (7.52)
                             2        2
                               ˆ
               In this expression, I 0 ( ) is the squared modulus of the optical field at
               frequency  .
                 The use of the Dirac delta function of Eq. (7.52) permits us to eval-
               uate the spectral radiance function of Eq. (7.33); it gives

                                          m   2      m
                                               ˆ
                               r
                             B(  s , 0, ˆ n,  ) =  I 0 ( ) =  ˆ I 0 ( )  (7.53)

                                           2
                 Since the noncoherent source is assumed to be spatially stationary,
                                                                  r
               the spectral radiance is independent of the average variable   s .
                 The spectral radiant power is
                                           2
                                                ˆ
                                      ( ) =  A· I 0 ( )             (7.54)
                                           3
               The spectral radiant exitance is given by
                                               2  ˆ
                                      r
                                    M(  s , 0,  ) =  I 0 ( )        (7.55)
                                               3
               Finally, the spectral radiant intensity takes the form
                                               A
                                                 ˆ
                                              2
                                    J ( ˆ n,  ) = m  I 0 ( )        (7.56)
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