Page 122 - Process Modelling and Simulation With Finite Element Methods
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Multiphysics                      109

          Here, the dependent variables are described as follows: u is the velocity vector, p
          is the pressure, and T is the temperature.  The independent variables are spatial
          coordinates (implied in the differential operators) and time t.  Everything else is
          a parameter ( V, p, a, K, g) with fixed value once the fluid and venue are selected.
          If there is no imposed moving boundary or pressure gradient, then the whole of
          the motion is created by  temperature gradients and is termed buoyant  (or free)
          convection.  If  there  are  imposed  velocities  or  pressure  gradients,  then  the
          application is termed forced convection.  Either case can be studied by the same
          multiphysics mode created in FEMLAB, but are historically considered different
          physical modes.
             In buoyant convection, there are two dimensionless parameters that govern the
          dynamical similarity of the problem, the Prandtl number that is a function of  the
          fluid, and the Rayleigh number that gives the relative importance of  temperature
          driving forces to dissipative mechanisms:
                                       V
                                  Pr = -
                                       K
                                        ag (V’                         (3.2)
                                  Ra =
                                           PVK

          where h is the depth of the fluid, 6T is the applied temperature difference, a is
          the coefficient of thermal expansion, g is the gravitational acceleration vector (g
          is its magnitude), p is the density, v the kinematic viscosity, and K is the thermal
          diffusivity  .
             Batchelor  [2]  showed  that  differentially heating  any  sidewall automatically
          induces buoyant motion, so the canonical buoyant convection problem is the hot
          walllcold wall  cavity flow.  This problem is always taken as a test case for the
          development of new numerical methods for transport phenomena. We will develop
          a FEMLAB model for it in this section.  This problem is treated in  [3], but the
          variations on the theme treated here are original.
          Launch FEMLAB and in the Model Navigator, select the Multiphysics tab.

                 Model Navigator
                        Select 2-D dimension
                        Select Physics modes-Incompressible  Navier-Stokes >>
                        Select ChE =Convection  and conduction >>
                        Select PDE modes 3 Coefficient form >>
                        OK
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