Page 508 - Bird R.B. Transport phenomena
P. 508

488  Chapter 16  Energy Transport by Radiation

                           the  "bulk  properties"  of  an enclosure containing radiation; quantum mechanics is  neces-
                           sary  in order  to describe  in  detail  the atomic and  molecular  processes  that occur  when
                           radiation  is  produced  within  matter  and  when  it  is  absorbed  by  matter; and  statistical
                           mechanics  is  needed  to describe  the way  in which  the energy  of  radiation  is  distributed
                           over  the wavelength  spectrum.  All  we  can do  in this elementary  discussion  is  define  the
                           key  quantities  and  set  forth  the  results  of  theory  and  experiment.  We  then  show  how
                           some  of  these  results  can  be  used  to  compute  the  rate  of  heat  transfer  by  radiant
                           processes  in simple  systems.
                               In  §16.1  and  §16.2  we  introduce  the  basic  concepts  and  definitions.  Then  in  §16.3
                           some  of  the principal  physical  results  concerning black-body  radiation are given.  In the
                            following section, §16.4, the rate  of heat exchange between  two black bodies  is  discussed.
                           This  section  introduces  no  new  physical  principles,  the  basic  problems  being  those  of
                            geometry.  Next,  §16.5  is  devoted  to  an  extension  of  the  preceding  section  to  nonblack
                           surfaces.  Finally, in  the  last  section, there  is  a  brief  discussion  of  radiation  processes  in
                            absorbing  media.  3


      §16.1  THE SPECTRUM OF ELECTROMAGNETIC RADIATION
                            When  a  solid  body  is  heated—for  example, by  an  electric  coil—the  surface  of  the  solid
                            emits radiation  of wavelength  primarily  in the range  0.1 to  10 microns. Such radiation  is
                            usually  referred  to as thermal radiation.  A quantitative description  of the atomic and mol-
                            ecular  mechanisms  by  which  the radiation  is  produced  is  given  by  quantum mechanics
                            and  is  outside  the scope  of  this  discussion.  A  qualitative  description, however,  is  possi-
                            ble:  When  energy  is  supplied  to  a  solid  body,  some  of  the  constituent  molecules  and
                            atoms are raised  to "excited  states/' There is a tendency for  the atoms or molecules  to re-
                            turn  spontaneously  to  lower  energy  states.  When  this  occurs, energy  is  emitted  in  the
                            form  of electromagnetic radiation. Because the emitted radiation results  from  changes  in
                            the  electronic, vibrational, and rotational states  of the atoms and molecules, the radiation
                            will be distributed  over  a range  of  wavelengths.
                               Actually,  thermal radiation represents  only a small part  of the total spectrum  of  elec-
                            tromagnetic radiation. Figure  16.1-1 shows roughly  the kinds  of  mechanisms that are re-
                            sponsible  for  the various  parts  of  the radiation spectrum. The various  kinds  of  radiation
                            are distinguished  from  one another only  by  the range  of  wavelengths  they include. In a
                            vacuum,  all  these  forms  of  radiant  energy  travel  with  the  speed  of  light  c. The  wave-
                            length  Л, characterizing an electromagnetic wave, is then related  to its frequency  v by  the
                            equation

                                                              A = %                             (16.1-1)

                            in  which  с  =  2.998  X  10 8  m/s.  In the visible  part  of  the  spectrum,  the  various  wave-
                            lengths are associated  with  the "color"  of the light.
                               For  some purposes,  it is convenient to think of  electromagnetic radiation from  a cor-
                            puscular point of view. Then we  associate with an electromagnetic wave  of frequency  v a
                            iphoton,  which  is a particle with  charge zero and mass  zero with  an energy  given  by
                                                              e  = hv                           (16.1-2)




                               3  For additional information on radiative heat transfer  and engineering  applications, see the
                            comprehensive  textbook by R. Siegel and J. R. Howell, Thermal Radiation Heat Transfer, 3rd edition,
                            Hemisphere Publishing Co., New York  (1992). See also J. R. Howell and M. P. Mengoc,, in Handbook of
                            Heat Transfer, 3rd edition, (W. M. Rohsenow, J. P. Hartnett, and Y. I. Cho, eds.), McGraw-Hill, New York
                            (1998), Chapter 7.
   503   504   505   506   507   508   509   510   511   512   513