Page 363 - Bird R.B. Transport phenomena
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§11.4  Use of the Equations of Change to Solve  Steady-State Problems  345

                               Porous spherical  shells               Fig. 11.4-1.  Transpiration cooling. The
                                                                      inner sphere is being  cooled by means
                                                                      of a refrigeration  coil to maintain its
                                                                      temperature at T . When  air is  blown
                                                                                    K
                                                                      outward, as shown, less refrigeration  is
                                                                      required.














                                            Air  flow out



      SOLUTION             We  postulate that for  this system  v  = Si>(r), T = T(r), and & =  ). The equation of continuity
                                                            r
                                                           r
                           in spherical coordinates then becomes
                                                            U                                  (11.4-21)
                                                            dr
                           This equation can be integrated  to give

                                                          2                                    (11.4-22)
                                                                      4тг
                                                         Y pV y  =  COnst.  =
                           Here w  is the radial mass flow rate of the gas.
                                 Y
                               The r-component of the equation of motion  in spherical coordinates is, from  Eq. B.6-7,
                                                     dv           d    d
                                                      r
                                                                                               (11.4-23)
                           The viscosity term drops out because  of  Eq. 11.4-21. Integration of  Eq. 11.4-23 then gives
                                                                      U-ff                     (11.4-24)
                                                                      L

                           Hence the modified  pressure  2P increases  with  r, but only very  slightly  for  the low  gas  veloc-
                           ity assumed here.
                               The energy equation  in terms  of  the temperature, in spherical  coordinates, is, according to
                           Eq. B.9-3,
                                                       C   dT      ^d_( dT\
                                                        p V   =  2  k  r2                      (11.4-25)
                                                          '  dr  r  dr\  dr j
                           Here we  have used  Eq. 11.2-8, for  which we  assume that the thermal conductivity  is constant,
                           the pressure  is  constant, and  there is  no viscous  dissipation—all  reasonable  assumptions  for
                           the problem at hand.
                               When  Eq.  11.4-22  for  the velocity  distribution  is used  for  v r  in  Eq. 11.4-25, we  obtain the
                           following  differential  equation  for  the temperature distribution  T(r) in  the gas  between  the
                           two  shells:
                                                        dT  _  4TT*  d  l 2 d T                (11.4-26)
                                                        dr   7n r  dr\  dr
                                                             w r C/
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