Page 126 - Physical Principles of Sedimentary Basin Analysis
P. 126

108                             Heat flow


                                        ∂T
                                 φ i   i c i  +   φ i   i c i v i  ·∇T −∇ · (λ∇T ) = S  (6.11)
                                        ∂t
                              i                 i
                 where the velocity of component i is the vector v i .
                   We will now look at temperature equation (6.11) for a porous medium, which is a
                 medium of two components: solid matrix and pore fluid. The coefficient before the term
                 ∂T/∂t is the weighted mean of   i c i for each component of the medium, using the volume
                 fractions φ i as normalized weights. The weighted mean of   f c f and   s c s is written as

                                          b c b = φ  f c f + (1 − φ)  s c s         (6.12)
                 where   b and c b are the bulk density and the bulk specific heat capacity, respectively.
                 Be aware that the notation   b c b hides the fact that we do not know each of these factors
                 separately, only their product.
                   The same averaging is carried out for the coefficient of the first-order term ∇T , assuming
                 that v i = v s for all components except the fluid (i = f ). It is done by replacing the fluid
                 velocity v f by the Darcy flux v D and the solid velocity v s . Recall from equation (2.31) that
                 the Darcy velocity is a volume flux measured relative to the velocity of the porous medium,

                                  v D = φ · (v f − v s )  or  φv f = v D + φv s .   (6.13)
                 The coefficient before the ∇T -term is therefore

                                 φ  f c f v f + (1 − φ)  s c s v s =   f c f v D +   b c b v s  (6.14)
                 and the temperature equation (6.11) becomes
                                      DT
                                    b c b  +   f c f v D ·∇T −∇ · (λ∇T ) = S        (6.15)
                                       dt
                 using the coefficients (6.12) and (6.14). Notice that time differentiation is written as a
                 material derivative with respect to the velocity of the (solid) sediment matrix.
                   The full temperature equation (6.15) is rarely needed, and most problems can be treated
                 with a simplified version. The most common simplifications apply to problems in 1D with
                 no source term for heat generation (S = 0) and where there is no heat convection (v D = 0).
                 Furthermore, we rarely have to deal with problems where the solid material is moving. The
                 material derivative therefore becomes the normal partial derivative, and the temperature
                 equation simplifies to
                                                         2
                                           ∂T       λ  
  ∂ T
                                              −             = 0                     (6.16)
                                           ∂t       b c b  ∂z 2
                 in the vertical direction. The only parameter left in the temperature equation is the thermal
                 diffusivity κ = λ/(  b c b ). Furthermore, we can make a dimensionless version of the equa-
                 tion if there is a characteristic length l 0 and a characteristic temperature T 0 in the problem.
                 Introducing the dimensionless quantities
                                           z        T            t
                                                ˆ
                                                             ˆ
                                       ˆ z =  ,  T =    and t =                     (6.17)
                                           l 0      T 0          t 0
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