Page 168 - Fundamentals of Computational Geoscience Numerical Methods and Algorithms
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158  7  Simulating Thermal and Chemical Effects of Intruded Magma Solidification Problems

                                                (x I , y I ) ∈ Γ RM ,     (7.4)
                             T R = T M

                    ∂T R     ∂T R         ∂T M     ∂T M
              λ R n x   + n y     − λ M n x    + n y
                     ∂x      ∂y            ∂x       ∂y
                                                                          (7.5)

                                          ∂x I    ∂y I
                = ρ M [L + c pM (T IM − T m )] n x  + n y  (x I , y I ) ∈ Γ RM ,
                                           ∂t      ∂t
            where x I and y I are the x and y coordinate components of the interface position;
            n x and n y are the x and y components of the unit normal to the interface between
            the rock and intruded magma; T IM is the temperature of the intruded magma; T m
            is the solidification temperature of the intruded magma; L is the latent heat of
            fusion of the intruded magma; Γ RM is the interface between the rock and intruded
            magma.
              Except for the boundary conditions on the interface between the rock and
            intruded magma, the boundary conditions on the other boundaries of the rock
            domain and intruded magma domain can be either of the Dirichlet, Neumann or
            mixed type (Carslaw and Jaeger 1959, Crank 1984, Alexiades and Solomon 1993,
            Zhao and Heinrich 2002). Since the boundary conditions on the other boundaries of
            the rock domain and intruded magma domain are trivial, it is not necessary to repeat
            them here.
              In order to develop an efficient and effective numerical algorithm for dealing with
            solidification of intruded magma in sills and dikes, it is necessary to introduce some
            related concepts. As shown in Fig. 7.1, supposing the initial position of the interface
            between the magma and rock is at position 1, the interface moves to position 2
            due to magma solidification during a time period, Δt M . As a result, the magma
            solidification thickness is expressed by ΔL M . If the length of the interface front is
            ΔL R , then the magma solidification area is the product of ΔL M and ΔL R during
            the time period Δt M . Since heat and volatile fluids are only released during magma
            solidification, we may consider the released heat and volatile fluids either as surface
            heat and mass sources in a two-dimensional problem or as volumetric heat and mass
            sources in a three-dimensional one. This means that it is physically possible to use



                                Position 1   Position 2
                                                   Magma
                              Rock                             Δ L
                                                                  R
                                           Interface movement
                                               direction

                                       Δ L
                                          M


            Fig. 7.1 Basic concepts related to the magma solidification problem
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