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Incompressible

                            Navier—Stokes                  Equations

















         11.1  Introduction

         The  solution  of the  incompressible  Navier-Stokes  equations  is discussed  in  this
         chapter  and  that  of  the  compressible  form  postponed  to  Chapter  12.  It  may
         appear  logical  to  consider  the  two  together  and  this  can  be  done  readily  to
         the  boundary  layer  equations,  where  the  equation  representing  conservation  of
         energy  has  to  be  added  to  complete  the  compressible  form.  The  differences  be-
         tween  the  incompressible  and  compressible  form  of the  Navier-Stokes  equations
         are  greater,  the  continuity  equation  for  the  former  is  elliptic  but  is  hyperbolic
         in  space  and  parabolic  in  time  for  the  latter.  These  differences  are  discussed
         in  more  detail  in  Section  11.2,  and  the  influence  of  the  equation  type  on  the
         boundary  conditions  are  discussed  in  Section  11.3.
            Once  the  equations  and  boundary  conditions  have  been  formulated,  a  solu-
         tion  algorithm  is  required.  There  are  several  numerical  methods  with  which  to
         solve the incompressible Navier-Stokes  (INS) equations, and they can be  divided
         in  two  classes.  The  first  class  uses  the  stream  function  variable  to  ensure  that
         the  conservation  of  mass  is  satisfied  and  this  approach  is  well-established  with
         two-dimensional  equations, but  extension to three-dimensions  is not  straightfor-
         ward  since the  stream  function  scalar  has to  be  replaced  by  a  three-dimensional
         vector  potential,  which  typically  is the  vorticity  vector.  Thus, the  modified  sys-
         tem  of  equations  contains  six  variables  as  opposed  to  the  four  variables  in  in-
         compressible  Navier-Stokes  equations  expressed  in  primitive  variables,  which
         corresponds  to  the  second  class  of  solution  methods.
            The  Marker  and  Cell  (MAC)  algorithm  developed  by  Harlow  and  Welch  [1]
         is an  early  method  with  which  to  solve  unsteady  equations.  It  uses  a  staggered
         grid  with  the  Poisson  equation  to  obtain  the  pressure  at  every  time  step.  The
         method  is  described  in  [2]  and  is  not  discussed  here.  Another  technique,  this
         time  mainly  for  steady  flows,  was  developed  by  Patankar  and  Spalding  [3]  and
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