Page 174 - Bird R.B. Transport phenomena
P. 174

158  Chapter 5  Velocity Distributions in Turbulent  Flow

                               Having  defined  the time-smoothed  quantities  and  discussed  some  of  the  properties
                           of  the fluctuating  quantities, we  can now  move  on to the time-smoothing  of  the equations
                           of  change.  To  keep  the  development  as  simple  as  possible,  we  consider  here  only  the
                           equations  for  a  fluid  of  constant density  and  viscosity. We  start by  writing  the  equations
                           of  continuity and motion with  v  replaced  by  its equivalent  v  + v'  and p by  its  equivalent
                           p + p'.  The equation  of continuity is then  (V • v)  = 0, and we  write the x-component of the
                           equation  of  motion, Eq. 3.5-6, in the д/dt  form  by using  Eq. 3.5-5:
                                                            (5 + v
                                                                     +
                                                                           +
                                                   +
                                                       +
                                              h  ъ  ^  % v '*>  iz ъ  ^         = °            (5 2 4)
                                                                                                -"
                                | p ( v  + v' )  = - £ ( ? + P') -  [ £ Р &  + v' ){v  + v' ) + -^ {v  + v' )(v  + v' )
                                    x    x                     Х    x  x   x    9  v    y  x    x
                                            +  ^ (v +  vl)(v  + v' )J  + pN {v  + v' )  + pg    (5.2-5)
                                                                      2
                                                 P  2    x    x         x    x     x
                           The  y-  and  z-components  of  the  equation  of  motion  can  be  similarly  written.  We  next
                           time-smooth these equations, making  use  of the relations given in Eq. 5.2-3. This gives







                                                                                                (5-2-7)

                           with  similar  relations  for  the y- and  z-components  of  the equation  of  motion. These  are
                           then  the time-smoothed equations  of continuity and motion for  a  fluid  with  constant  density
                           and  viscosity.  By  comparing  them  with  the  corresponding  equations  in  Eq.  3.1-5  and
                           Eq.  3.5-6  (the latter rewritten  in terms  of  д/dt),  we  conclude that
                               a.  The equation  of  continuity is the same  as we  had previously,  except  that v  is  now
                                 replaced  by  v.
                               b.  The equation  of motion now has v and p where  we  previously  had v and p. In ad-
                                 dition there appear the dashed-underlined  terms, which  describe  the momentum
                                 transport associated  with  the turbulent  fluctuations.
                               We  may  rewrite  Eq. 5.2-7 by  introducing the turbulent momentum  flux  tensor т  ш  with
                           components
                                          -<f>  ^rn    - ш  ^r^i     - ( 0  ^ r i  ^ ^
                                             =            =            =         g o  o n      ( 5  2 g )
                           These quantities  are usually  referred  to as  the Reynolds stresses.  We  may  also  introduce a
                           symbol  T {V)  for  the time-smoothed  viscous momentum flux. The components  of  this ten-
                           sor  have  the same  appearance  as  the expressions  given  in Appendices  B.I  to  B.3,  except
                           that the time-smoothed  velocity  components appear  in them:




                           This enables  us  then to write  the equations  of change in vector-tensor  form  as
                                                   (V  •  v)  = 0  and  (V  •  v )  = 0        (5.2-10,11)
                                                                          1
                                                                                ( 0
                                            j  t  pv  =  -Vp  -  [V  •  pv  v]  -  [V  • (т (у)  +  T )]  + pg  (5.2-12)
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