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,,M      Turbulence              Models














         3.1  Introduction

         The  Reynolds-averaged  equations  of  Section  2.3 and their  reduced  forms  in
         Section  2.4  cannot  be solved  without  information  about  the  various  correlation
         terms  that  make  up the stress  tensor,  and the same  is true  for the energy
         equation. It is well known  that  these terms,  which  represent  turbulent  diffusion,
         are  much  larger  than  those  corresponding  to laminar  diffusion  except  in  the
         immediate  vicinity  of a wall,  and  in turbulent  wall boundary  layers,  wakes,  jets
         and more complex  flows, these turbulent  diffusion  terms are  of similar  magnitude
         to  the  convective  terms.
            This  chapter  presents  a  brief  description  of various  models  to address the
         closure  problem  of turbulence  modeling.  The  subject  has been  studied  exten-
         sively in the  past  three  decades  and  useful  reviews  have  been  provided  in many
         journal  articles  and  in several  books,  see  for example,  Wilcox  [1], Cebeci  [2,3],
         Durbin  and  Reif  [4]. For  a detailed  description  of turbulence  models  and  their
         accuracy,  the  reader  is referred  to these  books.
            Early  approaches  to turbulence  modeling  include the mixing  length,  £,  as-
         sumptions  of Prandtl  [5] and  eddy-viscosity,  £ m ,  assumptions  of Boussinesq [6]
         for  wall boundary  layers and jets. Kolmogorov  [7] and Rotta  [8] proposed  models
         based  on partial-differential  equations  but,  in the  absence  of digital  computers,
         could  not  solve  them.  The  early  models  provided  a foundation  which  is still in
         use  today.  For  example,  the  concepts  of a mixing  length,

                                      QU'V'  =  6f  r ^ \                     (3.1.1)


         and  eddy-viscosity  expressions  of the  form
                                                   0H
                                           1
                                     -  QU'V  =  ge m—                      (3.1.2)
                                                   dy
         have  been  used  in the  vast  majority  of publications  concerned  with  turbulence
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