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64                                                 2.  Conservation  Equations




                                   St  =   ,„  ^  „  ,                    (2.4.39b)
                                               -
                                        QCp(T w    T e)u e
         Whereas the integration  of boundary-layer  equations  across the shear  layer  leads
         to  ordinary  differential  equations  that  are  much  easier  to  solve  than  partial-
         differential  equations,  their  solutions  require  auxiliary  equations.  The  momen-
         tum  integral  equation  has three  unknowns,  #,  H  and  cj, and  the  energy  integral
         equation  has two unknowns,  6T and  St; their  solutions require  at  least  two  other
         equations  to  solve  the  momentum  equation  and  one  for  the  energy  equation.
         While  there  are  several  useful  integral  methods  developed  for  two-dimensional
         flows  that  require  much  less computer  time  than  the  differential  methods,  they
         are limited  to simple  flows  [3, 7]. These limitations  are not  present  in  differential
         methods  and,  although  the partial  differential  form  of the  boundary-layer  equa-
         tions  is  more  difficult  to  solve,  its  use  is  preferred  in  this  book  and  in  current
         engineering  practice  and  the  solution  procedures  are  described  in  some  detail
         in  Chapter  7.


         2.5  Stability  Equations


        As  will be  explained  in  detail  in  Chapter  8,  a turbulent  boundary  layer  can  de-
        velop from  a laminar boundary  layer by the gradual  amplification  of  infinitesimal
        disturbances  within  the  boundary  layer  or  introduced  from  the  external  flow  or
        by  imperfections  in  the  body  surface.  At  first  these  disturbances  are  so  weak
        that  they  have  practically  no  influence  on  the  mean  flow  but  they  gradually
        increase  until  the  flow  is  distorted  and  the  fluctuating  velocity  and  pressure
        characteristics  of turbulent  flow  appear.  Transition  can  result  from  the  growth
        of  these  disturbances  in  the  boundary  layer  and  takes  place  over  a  streamwise
        distance  that  depends  on  the  boundary  conditions.
           The  behavior  of  these  disturbances  within  a  laminar  boundary  layer  can
        be  studied  by  small-disturbance  theory,  as  will  be  discussed  briefly  in  this  sec-
        tion  and  in  more  detail  in  Chapter  8.  To  derive  the  stability  equations  for
        two-dimensional  mean  flows with  two-dimensional  disturbances,  assume that  u,
        v  and  p  in  the  two-dimensional  form  of  Eqs.  (2.2.1)  to  (2.2.3)  represent  the
        instantaneous  components  of  the  flow  properties  and,  as  in  the  discussion  of
        turbulence  in  Section  2.3, these  components  are  divided  into  a  mean-flow  term
        and  a  fluctuating  term  so that  the  instantaneous  velocity  components  are  u + v!
                                                      f
        and  v +  v r  and  the  instantaneous  pressure  is p + p .  The  mean-flow  velocity  and
        pressure  terms  satisfy  the  boundary-layer  equations  for  a  steady  laminar  flow
        given  by Eqs.  (2.4.33)  and  (2.4.34)  with the  Reynolds  stress term  neglected  and
        with  overbars  on  u,  v  and  p.
           Next  consider  Eqs.  (2.2.1) to  (2.2.3)  with  instantaneous  velocity  components
        and pressure expressed  in terms  of their mean and  fluctuating  components.  Since
         1
        u ', v'  and  p'  are small, their  squares  and  products  can  be  neglected.  Noting  that
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