Page 209 - Fundamentals of The Finite Element Method for Heat and Fluid Flow
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CONVECTION HEAT TRANSFER
                                             l
                                              3
                                                                 A 4 l 4                      201
                                                     A 3
                                                                                Node
                                              A                     A 5
                                               2
                                                                          l 5
                                      l 2
                                                        A 1

                                                    l 1

                                      Figure 7.13 Two-dimensional linear triangular element


                           Often, it may be necessary to multiply the time-step  t by a safety factor due to
                        different methods of element size calculations. A simple procedure to calculate the element
                        size in two dimensions is

                                      2Area i
                             h = min         ,i = 1, number of elements connected to the node  (7.121)
                                        l i
                        where Area i are the area of the elements connected to the node and l i are the length of
                        the opposite sides as shown in Figure 7.13. For the node shown in this figure, the local
                        element size is calculated as

                                          h = min(A 1 /l 1 ,A 2 /l 2 ,A 3 /l 3 ,A 4 /l 4 ,A 5 /l 5 )  (7.122)
                           In three dimensions, the term 2Area i is replaced by 3Volume i and l i is replaced by the
                        area opposite the node in question.



                        7.6 Characteristic-based Split (CBS) Scheme

                        It is essential to understand the characteristic Galerkin procedure, discussed in the previous
                        section for the convection–diffusion equation, in order to apply the concept to solve the real
                        convection equations. Unlike the convection–diffusion equation, the momentum equation,
                        which is part of a set of heat convection equations, is a vector equation. A direct extension
                        of the CG scheme to solve the momentum equation is difficult. In order to apply the
                        characteristic Galerkin approach to the momentum equations, we have to introduce two
                        steps. In the first step, the pressure term from the momentum equation will be dropped
                        and an intermediate velocity field will be calculated. In the second step, the intermediate
                        velocities will be corrected. This two-step procedure for the treatment of the momentum
                        equations has two advantages. The first advantage is that without the pressure terms, each
                        component of the momentum equation is similar to that of a convection–diffusion equation
                        and the CG procedure can be readily applied. The second advantage is that removing the
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