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52                                                 2.  Conservation  Equations


         the  grid  spacing  in  the  curvilinear  space  is  uniform  and  of  unit  length,  that  is
         Arj  =  1,  Z\£  =  1.  This  produces  a  computational  space  £,r/  with  a  rectangular
         domain  and  with  a  regular  uniform  mesh  so that,  as  we shall  see  in  Section  6.3,
         the  differencing  schemes  used  in  the  numerical  formulation  are  simpler.  The
         original  Cartesian  space  is usually  referred  to  as  the  physical  domain.
            Using  the  chain  rule  of  differential  calculus,  we  can  write

                    d  _  d    <9  <9£  d  drj  d    d  .   d
                   ~di  =  lh  +  dZ~di  ^Fq'di
                    d     d  d£   d  dri   d  _   d
                   —   —     -  H       =  —ix  H   Vx                     (2.2.35)
                   dx    dt; dx  drj dx   <9£    drj
                    d_  _  d_d^    JL^R-J^c        A
                   dy  ~  d£dy  +  dr)dy~  dC y  +  dr} Vy
         or  in  compact  form  as
                                    d                d
                                   dt      1  6  Vt\ dr
                                    d                d
                                        =  0  £x  Vx\                     (2.2.36)
                                   dx
                                    d      0  Sy  Vy\  d
                                   dy              1  drj
            In  a  similar  manner,  the  second  derivatives  that  appear  in  the  momentum
         and  energy equations  can  be expressed  in transformed  variables. They  are,  how-
         ever, somewhat  more  involved  than  those  in Eq.  (2.2.35).  For  example,  with  the
         chain  rule,  it  can  be  shown  that

               d 2    d        0       d 2      d 2       d 2
                                        v_c2
                                       o/-9Sx
               dx 2    d^' xx  +  QiV. ] XX  I  d^ x  ' '  dr, 271x  +  2  drjd£,  Vx<,x
                      d_       d_      &  2    &_  2   0  d 2
                              dj]
               dy 2   d^yy  > nyy    .  ^ 2 s j ,  •  Qr)2  drjd£
                              drj
               d 2    d        d       d 2       d 2         d 2
                                71
             dxdy     d^ xy  +  drj ^  +  ap^ v  +  d7] 2r]xJ]v  +  dridt  (Vx£y +  ixVy)
                                                                          (2.2.37)
         In  terms  of  the  transformation  defined  by  Eq.  (2.2.34),  the  vector  form  of  the
         transformed  Navier-Stokes  equations,  Eq.  (2.2.30),  can  be  written  as
                  dQ     dQ      dQ      dE      dE    f  dF     dF


                          i     dE v     dE v     dF v      dF v          (2.2.38)
                          Re           Vx-?rr+ty-^-+Vy      dr]
                                                   di
                                          drj
            The  coefficients  of the  derivatives  in Eq.  (2.2.35)  with  respect  to  £,  77, namely
         £,t,£,x,£,y,Vt, Vx and  f] y are metric terms which can be obtained  from  the  transfor-
         mation  given  by Eq.  (2.2.34).  If the  relations  between the  independent  variables
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