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56                                                 2.  Conservation  Equations

            Q             + 2 +efy            e {v u ]       {v 2)     Q v w,)     (234)
              wt  = -% ^ "                ~ t ' ''       % '  - h'                  --



            e^   = -f z+  MV «) + oh -  e ^ ( w )  -  Q^tvft)  -  Q§-J^)   (2-3-5)
                             2

                 T~V/-T-I               r\          r\           r\
                              2
              gc p—  =q w  +  kV T  -  QC P—TW  -  gc p—TQ  -  Qc p—TW      (2.3.6)
         It  is  common  to  drop  the  overbars  on  the  basic  time  variables;  this  results
         in  a  continuity  equation  identical  to  that  given  by  Eq.  (2.2.1),  and  the  left-
         hand  sides  of  the  momentum  and  energy  equations,  Eqs.  (2.3.3)  to  (2.3.6),
         become  identical  to  the  equations  for  laminar  flow.  The  right-hand  sides  of  the
         momentum   and  energy  equations  also  resemble  the  right-hand  sides  of  Eqs.
         (2.2.2)  to  (2.2.4)  and  (2.2.11)  with  the  addition  of  the  Reynolds  normal,  shear
         stress, and  heat  flux  terms: in our previous notation  the Reynolds stresses  in  Eq.
         (2.3.3)  represent  the  turbulent  contributions  to  G XX,  a xy  and  a xz,  respectively.
         The  mean  viscous  contributions  are  still  given  by  Eq.  (2.2.7)  and  are  based  on
         the  mean-velocity  components.  Equations  (2.2.2)  to  (2.2.4)  thus  apply  to  both
         laminar  and  turbulent  flows,  provided  that  the  so-called  "stress  tensor",  cr^,
         including  the  viscous  contributions,  is written  as


                                 =  - ^      ^ _      ^ j                 (2.3.7a)
                              , y          +        +
        or
                                      (Tij =  4  +  4                     (2.3.7b)

        where  now  o\-  denotes  the  Reynolds  stresses  so  that  for  three-dimensional
                                    l
                                                                                /2
                        f2
                                                        l
                                                                       l
         floWS  a xx  =  -QU ,  (T xy  =  G yx  =  -QU'V , 1  G xz  =  (J zx  =  -Qu'w',  G yv  =  -  QV ,
             =     =  —QV'W',  l  — —QW' ,  and  G\-  is the  viscous  stress  tensor  as  given
                                       2
         <jy Z  a zy         a zz
        by  Eq.  (2.2.7)  for  a  Newtonian  fluid.
           We  note  that,  as  is the  case  for  the  momentum  equations,  additional  terms
         appear  on  the  right-hand  side  of  the  energy  equation,  (2.3.6).  These  terms,
        which  are the thermal  analogs  of the  Reynolds-stress  gradients  in Eqs.  (2.3.3)  to
                                                                         , f
         (2.3.5),  are  called  the  turbulent  heat-flux  gradients.  For  example.  gc pT v  is  the
        rate  of  flux  of enthalpy  in the  ^-direction  per  unit  area  in the  (x, z)  plane, due  to
        turbulent  fluctuations.  These  terms,  together  with  the  Reynolds-stress  terms  in
        the  momentum  equations,  introduce  additional  unknowns  into the  conservation
        equations.  To  proceed  further,  additional  equations  for  these  unknown  quanti-
        ties,  or  assumptions  regarding the  relationship  between  the  unknown  quantities
        to  the  time-mean  flow  variables,  are  needed.  This  is referred  to  as the  "closure"
        problem  in turbulent  flows:  we shall  discuss turbulence  modeling  in  some  detail
        in  Chapter  3.
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