Page 163 - Physical Principles of Sedimentary Basin Analysis
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6.11 Forced convective heat transfer           145

                                                 2 ˆ
                                           dT ˆ  d T
                                        v 0 ˆz  −    = 0                      (6.156)
                                           dˆz   dˆz 2
            where the velocity term is v 0 ˆz. The fluid flux is not constant but it decreases from v 0 at
                                                                ˆ
            the top (ˆz = 1) towards zero at the base (ˆz = 0). Setting f = dT /dˆz in the temperature
            equation (6.156) gives after integration that
                                       dT ˆ        1   2
                                          = c 1 exp  v 0 ˆz                   (6.157)
                                       dˆz         2
            and a second time of integration gives

                                            ˆ z    1
                                 ˆ                   2
                                T (ˆz) = c 1  exp  v 0 μ  dμ + c 2 .          (6.158)
                                          0      2
                                     ˆ
            The boundary conditions are dT /dˆz =ˆq at ˆz = 0 and T = 0at ˆz = 1. The first boundary
                                                        ˆ
            condition gives c 1 =ˆq and the second boundary condition gives
                                              1    1
                                   c 2 =−ˆq   exp   v 0 μ 2  dμ               (6.159)
                                            0     2
            and the solution for temperature becomes
                                              1     1
                                  ˆ
                                  T (ˆz) =−ˆq  exp  v 0 μ 2  dμ.              (6.160)
                                            ˆ z    2
            It is possible to rewrite solution (6.160) for the case where v 0 < 0 using the error-function
            defined as
                                           2     u      2
                                   erf(u) = √    exp(−μ ) dμ.                 (6.161)
                                            π  0
            The velocity v 0 is written as v 0 =−v 1 (where v 1 is positive) and the solution becomes


                                       π         v 1         v 1
                             T (ˆz) =ˆq    erf     ˆ z − erf      .           (6.162)
                             ˆ
                                      2v 1       2            2
            The scaled heat flux is ˆq =−1 in Figure 6.20 and the optimal values for v 1 are then
            v 1 = 1.07 and v 1 = 4.5. The parameter v 1 is the maximum of the linearly decreasing fluid
            flow term, and its optimal values are similar to the Pe-numbers obtained from the maximum
                                                                              ◦
                                                                   ◦
            vertical Darcy flow. Other numbers used in Figure 6.20 are T 1 = 0 C, T 2 = 33 C and
            z = 1000ˆz − 750 in units of meters. The temperature solution with units is therefore

                                                       z + 750
                                T (z) = T 1 + (T 2 − T 1 ) T ˆ                (6.163)
                                                        1000
            which is the analytical temperature plotted in Figure 6.20. The optimal value for v 1 can
            be used to estimate the Darcy flux, and we get that v 1 = 1.1 gives the Darcy flux v D =
                4
                                                     4
            1 · 10 mMa −1  and that v 1 = 4.5gives v D = 4 · 10 mMa −1 , assuming that l 0 = 1000 m
                            2 −1
            and κ = 3 · 10 −7  m s  .
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