Page 113 - Fundamentals of The Finite Element Method for Heat and Fluid Flow
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STEADY STATE HEAT CONDUCTION IN ONE DIMENSION
                                                   i
                                             T i
                                                              l         j  h, T a             105
                        Figure 4.3 Heat conduction through a homogeneous wall subjected to heat convection
                        on one side and constant temperature on the other. Approximation using a single linear
                        element


                        4.2.3 Finite element discretization

                        If we consider a typical homogeneous slab as shown in Figure 4.1, with nodes ‘i’ and ‘j’
                        on either side (see Figure 4.3), we can write

                                                     T = N i T i + N j T j                  (4.11)

                        where
                                                    x j − x         x − x i
                                               N i =       and N j =                        (4.12)
                                                    x j − x i       x j − x i
                           In local coordinates,
                                                           x         x
                                                  N i = 1 −  and N j =                      (4.13)
                                                           l          l
                        and the temperature derivative is
                                                dT     1    1
                                                   =− T i + T j
                                                dx     l    l

                                                        1 1   T i
                                                   = −            = [B]{T}                  (4.14)
                                                        l  l  T j
                        where l is the length of the element.
                           The elemental stiffness matrix (Chapter 3) is given as

                                                     T                  T
                                          [K] e =  [B] [D][B]d
 +   h[N] [N]dA s
                                                 
                A s

                                                    T                   T
                                              =   [B] [D][B]A dx +  h[N] [N]dA s            (4.15)
                                                 l                A s
                        where 
 is the volume integral, A s indicates surface area and h is the convective heat
                        transfer coefficient. After integration,

                                                    Ak x  1 −1         00
                                             [K] e =             + hA s                     (4.16)
                                                     l   −1   1        01
                        In a one-dimensional problem, [D] has only one entry, which is equal to k x .
                           Note that the convective heat transfer boundary condition is assumed to act on the right
                        face where N i = 0and N j = 1. This is the reason we have hA s added to the last nodal
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