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6.3  Finite-Difference  Method                                        183


         this  case,  the  solution  of  the  Laplace  equation  expressed  in  polar  coordinates,
         Eq.  (P2.19.2),  which  can  be  written  as

                                 ^    +  1 ^  +  1 ^  = 0                   (6.3.1)
                                 dr 2   r  dr  r 2  d6 2

         is  well  known,  see  for  example,  Anderson  [2].  For  a  cylinder  radius  of  r*o  and
         freestream  velocity  of  V^  (Fig.  6.3)  it  is  given  by

                                                     cos#
                                  =  Foorcos^  +  Kooro                     (6.3.2)























        Fig.  6.3.  Flow  over  a  circular  cylinder.


           The total  velocity  V  is composed  of radial  V r  and  circumferential  VQ velocity
        components  related  to  the  velocity  potential  4>  by

                                                   ldcf)
                                  V r         V e                          (6.3.3)
                                        dr'        r~d9
        The  solution  in  Eq.  (6.3.2)  obeys  the  boundary  conditions  at  the  body  surface
        and  at  infinity,  see Eqs.  (6.2.8)  and  (6.2.9),  which  in  our  case  can  be  written  as


                                     r  =  r 0 ,  *  0                    (6.3.4a)
                                              or
                                      oo,    -+  Vr^rcosO                 (6.3.4b)
           Before  we  discuss  the  numerical  solution  of  the  Laplace  equation  expressed
        in  polar  coordinates,  Eq.  (6.3.1),  it  is  useful  to  express  this  equation  and  its
        boundary  conditions  in  dimensionless  forms.  For  this  purpose,  define
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