Page 109 - Computational Fluid Dynamics for Engineers
P. 109

Numerical              Methods
                   for    Model          Parabolic

                   and      Elliptic         Equations

















         4.1  Introduction

         The  equations  of Chapters  2 and  3 are  of little  value  unless  they  can  be  solved.
         Since  known  analytical  methods  are  limited  to  some  special  flows  such  as  fully
         developed  laminar  flows  in ducts,  numerical  methods  are  required.  These  meth-
         ods  are  invariably  implemented  on  digital  computers,  so  this  chapter  provides
         an  introduction  to  computational  fluid  dynamics  and  to the  numerical  methods
         to  be  discussed  in  the  subsequent  chapters.
            The  numerical  solution  of  the  Navier-Stokes  and  Euler  equations  can  be
         obtained  by  using  finite-difference  and  finite-volume  methods.  Their  numeri-
         cal  solution  can  also  be  obtained  by  finite-element  methods.  However,  these
         methods  are  mainly  used  in  computational  structural  mechanics  and  are  yet
         to  gain  popularity  in  computational  fluid  dynamics.  Thus,  this  book  considers
         only  finite-difference  and  finite-volume  methods.  The  finite-difference  methods
         are  mainly  used  with  the  differential  form  of  the  conservation  equations,  and
         the  finite-volume  methods  are  used  in  conjunction  with  the  integral  form  of
         the  conservation  equations.  For  reduced  forms  of  the  Navier-Stokes  equations,
         such  as the  boundary-layer  equations  and  the  Orr-Sommerfeld  equation  which
         involve  the  numerical  solution  of  ordinary  and  partial-differential  equations,
         only  finite-difference  methods  are  considered.  The  finite-volume  methods  will
         be  considered  in  Chapter  12  in  connection  with  the  numerical  solution  of  the
         Navier-Stokes  and  Euler  equations  together  with  the  finite-difference  methods.
            Model equations  for the conservation  equations  are considered  in Section  4.2.
         These  equations  are  useful  to  "model"  the  behavior  of  the  more  complete  and
         complicated  partial-differential  equations  considered  in  subsequent  chapters.  In
         this  chapter  they  are  used  to  describe  the  numerical  solution  of  parabolic  and
         elliptic  equations  and  in the  following  chapter  the  numerical  solution  of  hyper-
         bolic  equations.
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