Page 135 - Introduction to Computational Fluid Dynamics
P. 135

P1: IWV
                                                                                   May 20, 2005
                                        0 521 85326 5
                                                                                                12:28
            0521853265c05
                           CB908/Date
                     114
                                                                 2D CONVECTION – CARTESIAN GRIDS
                            2. In incompressible flows, density is independent of pressure. Therefore, ρ l+1  =
                                 l
                               ρ = ρ (say). Derivation of the pressure-correction equation for compressible
                               flow is left to the reader as an exercise (see Date [15, 17]).
                            3. On staggered grids, the momentum equations are solved at the cell faces and,
                               therefore, residuals R uf1 and R uf2 must vanish at full convergence, rendering
                                ˙ m R = 0. Although this state of affairs will prevail only at convergence, one
                               may ignore ˙ m R even during iterative solution. Thus, effectively, the pressure-
                               correction equation applicable to computations on staggered grids is
                                               l+1           
            l+1
                                      1 ∂     ρ   r α V ∂p       1 ∂     ρ   r α V ∂p
                                                            m                          m
                                                               +
                                      r ∂x 1     AP  u f1  ∂x 1  r ∂x 2     AP  u f2  ∂x 2
                                            ∂(ρ l+1 )  1 ∂     l+1  l     1 ∂      l+1  l
                                          =        +         r ρ  u f1  +       r ρ  u f2  .   (5.32)
                                              ∂t      r ∂x 1             r ∂x 2
                               This equation is derived in [51] via an alternative route. It is solved with the
                               boundary condition



                                                          ∂p
                                                                = 0.                           (5.33)
                                                             m
                                                           ∂n
                                                               b
                               The explanation for this boundary condition is given in a later section.
                            4. On collocated grids, cell-face velocities must be evaluated by interpolation
                               to complete evaluation of ˙ m P because only nodal velocities u i are computed
                               through momentum equations. Thus, ˙ m P in Equation 5.30 is evaluated as

                                          
  l+1         l+1
                                     ˙ m P = ρ  r u  l    − ρ  r u  l     x 2
                                                   1 e         1 w
                                                                                         V
                                             
  l+1         l+1             
  l+1   o
                                          + ρ     r u  l    − ρ  r u  l     x 1 + ρ  − ρ   .   (5.34)
                                                     2 n          2 s         P      P
                                                                                         t
                               Now, to evaluate u i ,weuse multidimensional averaging rather than simple one-
                               dimensional averaging. Thus, for example,

                                                                          l          l
                                               1   1 
              x 2,n u 1,se  +  x 2,s u 1,ne
                                        u  l  =       u l  + u l  +                       ,
                                          1,e          1,P   1,E
                                               2   2                    x 2,n +  x 2,s
                                        u l  =  1 
 u l  + u l  + u l  + u l     ,
                                         1,se      1,P   1,E    1,S   1,SE
                                               4
                                        u l 1,ne  =  1 
 u l 1,P  + u l 1,E  + u l 1,N  + u l 1,NE     .  (5.35)
                                               4
                               Similar expressions can be derived for other interpolated cell-face velocities.
                            5. On collocated grids, we do not explicitly satisfy momentum equations at the
                               cell-face locations. Therefore, there is no guarantee that ˙ m R will vanish even at
   130   131   132   133   134   135   136   137   138   139   140