Page 556 - Bird R.B. Transport phenomena
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536  Chapter 17  Diffusivity  and the Mechanisms of Mass Transport

                            now multiply  each of  these expressions  by  the corresponding unit vector, add them, and
                            divide by  dS, we  get
                                                    PA^.Y  + Pa&yVy  + p b v  = p v              (17.7-5)
                                                                            a
                                                                     a z z
                            as the convective mass flux vector, which has units  of kg/m 2  •  s.
                               If one goes  back and repeats the story  of  the preceding paragraph, but using  every-
                            where molar units and the molar average velocity v*, then we  get
                                                    c<$ v*  + c b v*  + c b v*  = c v*          (17.7-6)
                                                       x    a y     Q z    a
                            as the convective molar flux vector, which has units of kg-mole/m 2  •  s.
                               To get the convective mass and molar fluxes  across  a unit surface  whose  normal unit
                            vector is n, we  form  the dot products (n • p v)  and  (n ° c v*),  respectively.
                                                                a
                                                                           a
      §17.8  SUMMARY OF MASS AND MOLAR FLUXES
                            In  Chapters  1 and  9 we  introduced the combined momentum  flux  tensor  ф  and  the com-
                            bined energy  flux  vector  e, which  we  found  useful  in  setting  up  the  shell  balances  and
                            equations  of  change, We  give the corresponding definitions  here for  the mass  and molar
                            flux  vectors.  We  add  together  the molecular  mass  flux  vector  and  the convective  mass
                            flux  vector  to get  the combined  mass flux vector, and  similarly  for  the combined  molar flux
                            vector:

                            Combined  mass      flux:      n a  = ) a  + p v                    (17.8-1)
                                                                    a
                            Combined molar       flux:     N a  = J* + c v*                      (17.8-2)
                                                                     a
                            In  the  first  three  lines  of  Table  17.8-1  we  summarize  the  definitions  of  the  mass  and
                            molar  fluxes  discussed  so  far.  In the shaded  squares  we  also  give the definitions  of  the
                            fluxes *  (mass flux with  respect  to the molar average  velocity)  and  j  u  (molar flux with  re-
                                 j
                            spect to mass average  velocity). These "hybrid"  fluxes  should normally not be used.
                               In  the remainder  of  Table  17.8-1 we  give  a summary  of  other useful  relations, such
                            as  the sums  of  the  fluxes  and  the interrelations among  the  fluxes.  By  using  Eqs.  (J) and
                            (M) we  can rewrite Eqs. 17.8-1 and 2 as
                                                                    N
                                                         ) a  = n a  -  (D  2  Щ                (17.8-3)
                                                                   a
                                                                    0=1
                                                         j :  = N  -  x  f  Щ                   (17.8-4)
                                                               a   A
                                                                    /3 = 1
                            When  simplified  for  binary  systems,  these  relations  can  be  combined  with  Eqs.  17.7-3
                            and  17.7-4, to get  Eqs.  (C) and  (D) of  Table  17.8-2, which  are equivalent  forms  of  Fick's
                            (first)  law.  The forms  given  in Eqs. (E) and  (F) of Table  17.8-2, in terms  of  the relative  ve-
                            locities  of the species, are interesting because they involve  neither v nor v*.
                               In  Chapter  18 we  will  write  Fick's  law  exclusively  in  the  form  of  Eq.  (D) of  Table
                            17.8-2.  It  is  this  form  that  has  generally  been  used  in  chemical  engineering.  In  many
                            problems  something  is  known  about  the  relation  between  N^  and  N  B  from  the  stoi-
                            chiometry  or  from  boundary  conditions. Therefore  N  can be  eliminated  from  Eq. (D),
                                                                          B
                            giving a direct relation between  N^ and Vx A  for  the particular problem.
                               In  §1.7 we  pointed out that the total molecular momentum flux through a surface  of
                            orientation n is the vector  [n •  IT]. In §9.7 we mentioned the analogous quantity for the mol-
                            ecular  heat  flux—namely,  the scalar  (n •  q). The analogous  mass  transport quantities  are
                            the scalars  (n • j )  and (n • J*), which give the total mass and molar fluxes through a  surface
                                         a
                            of  orientation n. Similarly,  for  the combined  fluxes  through a surface  of  orientation n,  we
                            have for momentum [n • ф], for energy  (n ° e), and for  species  (n • n )  and  (n • N ).
                                                                                                a
                                                                                     a
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