Page 527 - Bird R.B. Transport phenomena
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§16.6  Radiant Energy  Transport in Absorbing  Media  507

                            tive term in Eq. 16.6-2, since the photons move independently  of  the local material  veloc-
                            ity.  Note further  that the term {%  -  si)  appears  with  opposite  signs in  Eqs.  16.6-1  and  2,
                            indicating  that  a  net  gain  of  radiant  energy  occurs  at  the expense  of  molecular  energy.
                            Equation  16.6-2 can also be  written  for  the radiant energy  within  a frequency  range  v to
                            v  + dv\

                                                                  (
                                                       {
                                                    — и ?  = -(V  •  qj°)  + {%  -  si )         (16.6-3)
                                                                         v   v
                            This expression  is obtained  by  differentiating  Eq. 16.6-2 with  respect  to v.
                               For  the purpose  of  simplifying  the  discussion,  we  consider  a  steady-state  nonflow
                            system  in which  the radiation  travels  only  in the positive  z direction. Such  a system  can
                            be  closely  approximated  by  passing  a collimated  light  beam  through  a  solution  at  tem-
                            peratures  sufficiently  low  that the emission  by  the solution  is unimportant.  (If  emissions
                            were  important, it would  be  necessary  to consider  radiation  in  all  directions.)  These  are
                            the  conditions  commonly  encountered  in  spectrophotometry.  For  such  a  system,  Eqs.
                            16.6-1  and 2 become

                                                          0=~q     + s&                         (16.6-4)
                                                                z
                                                          П    u  (r)                           (16.6-5)
                                                          0  =  —j-qz  ~~  '
                            In  order  to  use  these  equations,  we  need  information  about  the  volumetric  absorption
                            rate si.  For a unidirectional beam  a conventional expression  is
                                                             si  =  m q (r)                     (16.6-6)
                                                                  a
                            in which  m  is known as the extinction  coefficient. Basically, this states  that the rate of pho-
                                     a
                            ton absorption  is proportional  to the concentration  of  photons.



       EXAMPLE   16.6-1     A  monochromatic radiant beam  of frequency  v, focused  parallel to the z-axis, passes through
                            an  absorbing  fluid. The local rate  of energy  absorption  is given by  m j$,  in which  m  is the
                                                                                                av
                                                                                   a
      Absorption  of  a     extinction  coefficient  for  radiation  of  frequency  v. Determine  the distribution  of the radiant
      Monochromatic         flux  q^(z) in the system.
      Radiant  Beam
                            SOLUTION
                            We  neglect  refraction  and scattering  of the incident beam. Also, we assume  that the liquid  is
                            cooled so that re-radiation can be neglected. Then Eq. 16.6-5 becomes for steady  state

                                                              d                                 (16.6-7)
                                                             ~d~z l

                            Integration with respect to z gives
                                                                                                (16.6-8)

                                                      2
                            This is Lambert's law of absorption,  widely used  in spectrophotometry. For any given pure ma-
                            terial, m  depends in a characteristic way on v. The shape of the absorption spectrum is there-
                                  av
                            fore a useful  tool for qualitative  analysis.



                                 J. H. Lambert, Photometria, Augsburg  (1760).
                               2
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