Page 510 - Bird R.B. Transport phenomena
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490  Chapter  16  Energy Transport by Radiation

      §16.2  ABSORPTION AND EMISSION AT SOLID             SURFACES
                           Having  introduced  the  concepts  of absorption  and  emission  in  terms  of  the  atomic  pic-
                           ture, we now proceed  to the discussion  of the same processes  from  a macroscopic  view-
                           point. We restrict the discussion here to opaque solids.
                               Radiation  impinging  on  the  surface  of  an  opaque  solid  is  either  absorbed  or  re-
                           flected.  The  fraction  of  the  incident  radiation  that  is  absorbed  is  called  the absorptivity
                           and  is given  the  symbol  a. Also  the  fraction  of  the  incident  radiation  with  frequency  v
                           that is absorbed  is designated by a v. That is, a and a v are defined  as
                                                        a  =      a  =
                                                           ^T)    »   \)                     (16.2-1,2)

                           in  which  cffdv  and  cftdv are the  absorbed  and  incident  radiation  per  unit  area  per  unit
                           time in the frequency  range  v to  v  + dv. For any  real body, a u will be less than  unity  and
                           will  vary  considerably  with  the  frequency.  A  hypothetical  body  for  which  a,, is  a  con-
                           stant, less than unity, over the entire frequency  range and  at all temperatures  is called a
                           gray body. That is, a gray body always absorbs the same fraction  of the incident  radiation
                           of all frequencies.  A limiting case of the gray body is that  for which a,, = 1 for all  frequen-
                           cies and  all temperatures. This limiting behavior defines  a black body.
                               All solid surfaces emit radiant energy. The total radiant energy emitted per unit  area
                                                      {e)
                           per unit time is designated  by q , and  that emitted  in the frequency  range  v to  v + dv is
                           called q^dv.  The corresponding rates  of energy emission from  a black body are given  the
                           symbols <$ and  q^dv.  In terms  of these quantities, the emissivity for  the total  radiant-en-
                           ergy emission as well as that  for a given frequency  are defined  as
                                                            n(e)
                                                        e =                                   (16.2-3,4)
                           The emissivity  is also a quantity  less than unity  for  real, nonfluorescing  surfaces  and  is
                           equal to unity  for black bodies. At any given temperature  the radiant  energy emitted  by
                           a  black  body  represents  an  upper  limit  to  the  radiant  energy  emitted  by  real,  nonfluo-
                           rescing  surfaces.
                               We  now  consider  the  radiation  within  an  evacuated  enclosure  or  "cavity"  with
                           isothermal walls. We imagine that the entire system is at equilibrium. Under  this condi-
                           tion, there is no net  flux  of energy across the interfaces between  the solid and  the cavity.
                           We now  show  that  the  radiation  in  such  a  cavity  is independent  of  the  nature  of  the
                           walls  and  dependent  solely  on  the  temperature  of  the  walls  of  the  cavity.  We  connect
                           two cavities, the walls  of which are at the same temperature, but are made  of two  differ-
                           ent materials, as shown in Fig. 16.2-1. If the radiation intensities  in the two cavities were
                           different,  there would be a net transport  of radiant  energy  from  one cavity to the  other.
                           Because such  a flux  would  violate the second  law  of thermodynamics,  the radiation  in-
                           tensities  in the two cavities must  be equal, regardless  of  the compositions  of  the  cavity
                           surfaces.  Furthermore,  it  can  be  shown  that  the  radiation  is  uniform  and  unpolarized
                           throughout  the cavity. This cavity radiation plays  an important  role  in the  development





                             Material 1     Material 2




                                                       Fig. 16.2=1,  Thought experiment  for proof  that cavity radi-
                                                       ation is independent  of the wall materials.
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