Page 29 - Fundamentals of The Finite Element Method for Heat and Fluid Flow
P. 29

SOME BASIC DISCRETE SYSTEMS
                        where h is the heat transfer coefficient and T a is the ambient temperature. We can rearrange
                        the previous three equations as follows:
                                                            k 1 A   k 1 A                      21
                                                               T 1 −   T 2 = qA
                                                            L 1     L 1
                                           k 1 A      k 1 A  k 2 A     k 2 A
                                         −    T 1 +     +      T 2 −   T 3 = 0
                                           L 1      L 1    L 2      L 2
                                                    k 2 A      k 2 A
                                                   −    T 2 +    + hA T 3 = hAT a           (2.11)
                                                     L 2      L 2
                           The above equation can be rewritten in matrix form as
                                       k 1 A    −k 1 A
                                                                   
                                                              0
                                       L 1       L 1                            
                                                                   
                                                                   
                                     −k 1 A  k 1 A  k 2 A  −k 2 A   T 1   qA 
                                                 +                         =    0           (2.12)
                                                                   
                                                                    T 2
                                     L 1     L 1   L 2      L 2               
                                                                    T 3       hAT a
                                                −k 2 A    k 2 A
                                    
                                                                   
                                        0                     + hA
                                                 L 2       L 2
                        or
                                                       [K]{T}={f}                           (2.13)
                           The solution of Equation 2.13 gives the unknown temperatures T 1 , T 2 and T 3 .Inthe
                        case of heat conduction, there is only one degree of freedom at each node as temperature
                        is a scalar. The following important features of Equation 2.13 should be observed.
                           • The characteristics of each layer of the slab for heat conduction can be written as
                                                   kA     1 −1          Q
                                                                T i
                                                                   =                        (2.14)
                                                   L   −1   1  T j     −Q
                           • where Q is the total heat flow and is constant.

                           • The global stiffness matrix [K] can be obtained by assembling the stiffness matrices
                             of each layer and the result is a symmetric and positive definite matrix.

                           • The effect of the heat flux boundary condition appears only in the loading terms {f}.
                           • The convective heat transfer effect appears both in the stiffness matrix and the loading
                             vector.

                           • The thermal force vector consists of known values. The method of assembly can be
                             extended to more than two layers of insulation.

                           • The effect of natural boundary conditions (flux boundary conditions) is evident at
                             the formulation stage.

                           In summary, if [K]and {f} can be formed, then the temperature distribution can be
                        determined by any standard matrix solution procedure.
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