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                                                                               1D HEAT CONDUCTION
                               Thus, A i and B i can be calculated by recurrence. The implementation steps are
                            as follows:
                                                                                        l
                            1. Prepare a i , b i , and c i for i = 2to N − 1 from knowledge of the T distribution.
                                                                                        i
                            2. From comparison of Equations 2.69 and 2.71, set A 2 = a 2 and B 2 = c 2 (because
                               b 2 = 0 via the boundary condition specification). Now evaluate A i and B i for
                               i = 3to N − 1 by recurrence using Equations 2.74 and 2.75.
                            3. Evaluate T i by backwards substitution using Equation 2.71, that is, from
                               i = N − 1 to 2. Note that since we prescribe boundary conditions such that
                               AE N−1 = 0, it follows that A N−1 = 0.
                            4. Evaluate fractional change as before and go to step 1 if the convergence criterion
                               is not satisfied.
                               The TDMA is essentially a forward elimination (implicit in the recurrence
                            relations) and backward substitution procedure in which temperatures at all i are
                            updated simultaneously in step 3. Hence, the TDMA is also called a line-by-line
                            procedure to contrast it with the point-by-point GS procedure introduced earlier.
                            Further, we note that if a i , b i , and c i were constants and not functions of T then
                            the TDMA would yield a solution in just one iteration whereas the point-by-point
                            procedure would require several iterations even when coefficients are constants.


                            2.8.3 Applications

                            To illustrate performance of the methods just described, we consider two steady-
                            state problems. 7

                            Problem 2 – Rectangular Fin [80]
                            A rectangular fin of length 2 cm, thickness 2 mm, and breadth 20 cm is attached
                            to a plane wall as shown in Figure 2.10. The wall temperature T w = 225 C
                                                                                                  ◦
                                                           ◦
                            and ambient temperature T ∞ = 25 C. For the fin material, k = 45 W/m-K and
                                                     2
                            the operating h = 15 W/m -K. Determine the heat loss from the fin and its
                            effectiveness. Assume the tip heat loss to be negligible.

                            Solution
                            The exact solution to this problem is
                                           coshm (L − x)             √
                                T − T ∞
                                        =               ,     Q loss =  hP k A (T w − T ∞ )tanh(mL),
                                              coshmL
                                T w − T ∞
                                                                                               (2.76)
                                       √
                            where m =    hP /kA. In our problem, perimeter P = 2 × 20 = 40 cm, area A =
                                           2
                            20 × 0.2 = 4cm , and L = 2 cm. Therefore, m = 18.257m −1  and Q loss = 23 W.

                            7  The USER files for these problems are given in Appendix B.
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