Page 218 - Fundamentals of The Finite Element Method for Heat and Fluid Flow
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CONVECTION HEAT TRANSFER
                        210
                        Step 1: Intermediate velocity calculation x 1 component
                                                                   n
                                                        n
                                                                              n
                                     [M]   {˜ u 1 }  =−[C]{u 1 } − [K m ]{u 1 } − [K s ]{u 1 } +{f 1 }  (7.158)
                                           t
                        and for the x 2 component
                                         {˜ u 2 }       n          n          n
                                     [M]      =−[C]{u 2 } − [K m ]{u 2 } − [K s ]{u 2 } +{f 2 }  (7.159)
                                           t
                        Step 2: Pressure calculation
                                               n     1
                                          [K]{p} =−     [G 1 ]{˜ u 1 }+ [G 2 ]{˜ u 2 } +{f 3 }  (7.160)
                                                      t
                        Step 3: Velocity correction
                                                    n+1                    n
                                             [M]{u 1 }  = [M]{˜ u 1 }−  t[G 1 ]{p}
                                                    n+1                    n
                                             [M]{u 2 }  = [M]{˜ u 2 }−  t[G 2 ]{p}         (7.161)
                        Step 4: Temperature calculation
                                           {T}          n         n         n
                                       [M]     =−[C]{T} − [K t ]{T} − [K s ]{T} +{f 4 }    (7.162)
                                            t
                           The above four steps are the cornerstone of the CBS scheme for the solution of the
                        heat convection equations. An extension of the above steps for solving the conservation
                        form and three-dimensional equations is straightforward. Interested readers should consult
                        some of the appropriate publications (Nithiarasu 2003; Zienkiewicz et al. 1999).
                           The mass matrix [M] used in the above steps may be ‘lumped’ to simplify the solution
                        procedure. This is an approximation, but a worthwhile and time-saving approximation. Mass
                        lumping will eliminate the need for the matrix solution procedure necessary for consistent
                        mass matrices. The lumped mass matrix for a linear triangular element is constructed by
                        summing the rows and placing on the diagonals. The elemental lumped mass matrix of a
                        linear triangular element is
                                                                        
                                                        40 0         10 0
                                                     A            A
                                             [M Le ] =   04 0   =   01 0               (7.163)
                                                    12            3
                                                        00 4         00 1
                           If the above mass lumping procedure is introduced into the CBS steps, some small
                        errors will occur in the transient solution. For steady state solutions, however, no errors
                        are introduced. However, for transient problems an accurate solution can still be obtained
                        by appropriate mesh refinement.



                        7.6.2 Time-step calculation

                        The time-step restrictions are very similar to the convection–diffusion equation (Equation
                        7.119). The local time step at each and every node can be computed as follows:

                                                     t = min( t c , t d )                  (7.164)
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