Page 97 - Fundamentals of The Finite Element Method for Heat and Fluid Flow
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THE FINITE ELEMENT METHOD
                        obey certain continuity and compatibility conditions. These conditions will be discussed
                        later in the text.
                                                            n
                                                                e  e                           89
                                                     I(T ) =   I (T )                      (3.248)
                                                            e=1
                           Thus, instead of working with a functional defined over the whole solution region, our
                        attention is now focused on a functional defined for the individual elements. Hence,
                                                           n
                                                               e
                                                     δI =    δI = 0                        (3.249)
                                                          e=1
                                           e
                        where the variation in I is taken only with respect to the r nodal values associated with
                        the element e,thatis,
                                            ∂I e     ∂I e
                                                 =     = 0 with j = 1, 2,... ,r            (3.250)
                                            ∂T      ∂T j
                           Equation 3.250 comprises a set of r equations that characterize the behavior of the
                        element e. The fact that we can represent the functional for the assembly of elements
                        as a sum of the functional for all individual elements provides the key to formulating
                        individual element equations from a variational principle. The complete set of assembled
                        finite element equations for the problem is obtained by adding all the derivatives of I,as
                        given by Equation 3.250, for all the elements. We can write the complete set of equations as
                                                 n    e
                                           ∂I       ∂I
                                              =        = 0 with i = 1, 2,... ,M            (3.251)
                                          ∂T i      ∂T i
                                                e=1
                           The problem is complete when the M set of equations are solved simultaneously for
                        the M nodal values of T . We now give the details for formulating the individual finite
                        element equations from a variational principle.
                                                     2           2          2
                                      1        ∂T  e       ∂T  e       ∂T  e
                                  e                                                e
                                 I =       k x       + k y       + k z       − 2GT   d
                                      2  
      ∂x          ∂y         ∂z

                                             e        1    e     2
                                     +     qT ds +      h(T − T a ) ds                     (3.252)
                                                      2
                                        S 2e        S 3e
                        with
                                                            
                                                          T 1
                                                            
                                                            
                               e                           T 2
                             T = [N]{T}= [N 1 ,N 2 ,... ,N r ]  = N 1 T 1 + N 2 T 2 + ··· N r T r  (3.253)
                                                         ...
                                                            
                                                            
                                                           T r
                        and
                                                        ∂T  e
                                                            = N 1
                                                        ∂T 1
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