Page 519 - Bird R.B. Transport phenomena
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§16.4  Direct Radiation Between  Black Bodies in Vacuo  at Different  Temperatures  499





























                             Dimension ratio  -

      Fig. 16,4-3.  View factors  for  direct radiation between  adjacent  rectangles  in perpendicular planes
      [H. C. Hottel, Chapter 3 in W. H. McAdams, Heat Transmission, McGraw-Hill, New York  (1954), p. 68].



                           where  Aj  and  A 2  are usually  chosen  to be  the total areas  of  bodies  1 and  2. The dimen-
                           sionless  quantities  F  and  F ,  called  view factors (or angle factors or configuration factors),
                                            u      2]
                           are given  by
                                                              COS  0]  COS  0 2
                                                                          dA dA               (16.4-10)
                                                                            x  2
                                                              COS  0,  COS  0 2
                                                                   12     dAdA 2              (16.4-11)
                                                                            l
                           and  the two view  factors  are related by  А ¥ и  = A F 2V  The view  factor F  represents  the
                                                              л
                                                                     2
                                                                                        12
                           fraction  of radiation leaving  body  1 that its directly intercepted by body  2.
                               The  actual  calculation  of  view  factors  is  a  difficult  problem,  except  for  some  very
                           simple  situations. In Fig.  16.4-3 and  Fig.  16.4-4  some view  factors  for  direct radiation are
                                  23 4
                           shown. '  When  such charts are available,  the calculations  of energy  interchanges by  Eq.
                           16.4-9 are easy.
                               In  the  above  development,  we  have  assumed  that  Lambert's  law  and  the
                           Stefan-Boltzmann  law  ma)f be used  to describe  the nonequilibrium transport process, in
                           spite  of the fact  that they are strictly  valid only  for  radiative  equilibrium. The errors thus
                           introduced  do  not seem  to have  been  studied  thoroughly, but  apparently  the  resulting
                           formulas  give a good  quantitative description.




                               2  H. С  Hottel and A. F. Sarofim, Radiative  Transfer, McGraw-Hill, New  York  (1967).
                               3  H.C. Hottel, Chapter 4 in W. H. McAdams, Heat Transmission,  McGraw-Hill, New  York  (1954).
                               4  R. Siegel  and J. R. Howell, Thermal Radiation Heat Transfer, 3rd edition, Hemisphere Publishing Co.,
                           New  York  (1992).
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