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3.4  Two-Equation  Models                                              89



            There  are  several  approaches  that  can  be  used  to  model  the  turbulence  ki-
         netic energy  and  rate  of dissipation  equations  near the  wall region.  For  example,
         in  one  approach,  wall  functions  are  introduced  into  Eqs.  (3.4.3)  and  (3.4.4)  so
         that  the  model  equations  are  applicable  throughout  the  whole  layer.  Launder
         and  Sharma  [18]  modify  Eq.  (3.1.4)


                                                k 2
                                       "1  =  0^—                           (3.4.6)
                                                 £
         and  rewrite  Eqs.  (3.4.3)  and  (3.4.4)  as


                                                                  1 2 2
                dk    dk     d  (u tdk\      fdu\ 2      n     fdk / ^
              U      V                    Ut              V
               dx     dy    dy\a kdyj       \dy)            \  dy  I

                                                                    2
           de    de     d  fu tde\      e  (du\ 2    £   e 2  n   (d u\ 2  , o  .


         where
                                           3.4               2
                           U  =  exp              2  ,  R t l  =  —        (3.4.9a)
                                      (l  + J 4 /50) J'     ve
                                           i
                                     =  l -  0.3exp(-i2?)                 (3.4.9b)
                                  f 2
           The  boundary  conditions  are


                                    y  =  0,  k  =  £ =  0               (3.4.10a)

                                 y  —>  6,  k  —> k e,  s  —>  e e        (3.4.10b)

         To  avoid  numerical  problems,  k e  and  £ e  should  not  be  zero.  In  addition,  k e  and
           can  not  be  prescribed  arbitrarily  because  their  development  is  governed  by
         £ e
        the  transport  equations  (3.4.7)  and  (3.4.8)  written  at  the  boundary-layer  edge,
                                         dk
                                       u e—-  =  -£ e                    (3.4.11a)







         The  above  equations  can  be  integrated  with  respect  to  x  with  initial  conditions
        corresponding  to  k eo  and  £ eo  at  XQ. The  solution  provides the  evolutions  of  k{x)
         and  e(x)  as  boundary  conditions  for  the  k-  and  ^-equations.
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