Page 526 - Bird R.B. Transport phenomena
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506  Chapter  16  Energy Transport by Radiation

       §16.6  RADIANT ENERGY TRANSPORT IN ABSORBING                 MEDIA   1
                            The  methods  given  in  the  preceding  sections  are  applicable  only  to  materials  that  are
                            completely transparent  or completely opaque. To describe energy transport  in nontrans-
                            parent  media,  we  write  differential  equations  for  the  local  rate  of  change  of  energy  as
                            viewed  from  both  the  material  and  radiation  standpoint.  That  is, we  regard  a  material
                            medium  traversed  by electromagnetic  radiation  as two  coexisting  "phases": a  "material
                            phase," consisting  of all the mass in the system, and  a "photon phase," consisting  of  the
                            electromagnetic  radiation.
                                In Chapter  11 we have already  given  an  energy balance equation  for  a system  con-
                            taining  no  radiation.  Here  we  extend  Eq.  11.2-1  for  the  material  phase  to  take  into  ac-
                            count  the  energy  that  is  being  interchanged  with  the  photon  phase  by  emission  and
                            absorption  processes:

                                                    • pUv)  -  (V  • q)  -  (V  • pv)  -  (T:VV)  -  {%  -  (16.6-1)

                            Here we have introduced  % and  si,  which are the local rates  of photon emission and  ab-
                            sorption  per unit volume, respectively. That is, % represents the energy lost by the mate-
                            rial  phase  resulting  from  the  emission  of  photons  by  molecules, and  su represents  the
                            local gain  of energy by the material phase resulting from photon absorption by the mole-
                            cules  (see  Fig. 16.6-1). The q  in  Eq.  16.6-1 is the conduction  heat  flux  given by  Fourier's
                            law.
                                For  the  "photon  phase,"  we  may  write  an  equation  describing  the  local  rate  of
                                                         (r)
                            change  of radiant energy density u :
                                                                         -si)                   (16.6-2)

                                     (r)
                            in which  q  is the radiant energy flux. This equation may be obtained by writing a radi-
                            ant energy balance on an element  of volume fixed  in space. Note that there is no convec-























                                                               Fig. 16.6=1.  Volume element over which energy
                                                               balances are made; circles represent molecules.




                                1
                                 G. C. Pomraning, Radiation Hydrodynamics, Pergamon Press, New  York (1973);  R. Siegel  and
                            J. R. Howell, Thermal Radiation Heat Transfer, 3rd edition, Hemisphere Publishing Co., New  York  (1992).
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