Page 192 - Process Modelling and Simulation With Finite Element Methods
P. 192

Simulation and Nonlinear Dynamics         179

          the problem can be found in Drazin and Reid [5]. The gist of the problem is that
          a vertically decreasing temperature profile and no flow is identically a solution to
          the boundary value problem stated as
                         au
                         -+u.VU  = ---Vpi-vV2~+-T
                                        1
                                                      ag
                          at            P              P
                         v.u = 0


                          dt
          (c.f. equations 3.1) with boundary conditions of


                                                                       (5.7)


          where the bottom temperature  is usually greater than the top.  The dimensionless
          groups that matter are still the Prandtl number and the Rayleigh number:
                                       V
                                  Pr = -
                                       K
                                                                       (5.8)
                                       ag (ST) h3
                                  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, p
          is the density, v the kinematic viscosity, and K is the thermal diffusivity.
             You can be forgiven for thinking that we have just turned the hot wall-cold
          wall  problem  on  its  side.  In  the  case  of  vertical  heated  walls,  motion  is
          automatically  induced even with an infinitesimal  temperature  difference.  Fluid
          along  a  hot  vertical  wall  must  rise.  For  horizontal  heated  walls,  however,  a
          steady,  linear  temperature  profile  with  no  motion  is  an  exact  solution to  the
          system.  If  the heating is from above, that makes perfect  sense as hot light fluid
          will  lie over colder dense fluid  - gravity supplies a buoyant  restoring force to
          any fluid  element  that  might  be  displaced  vertically.  For heating  from below,
          however,  the  stratification  has  dense fluid  over  light.  Buoyant forces  should
          overturn this  top heavy  profile.  Yet, if  viscosity  and thermal  conductivity  are
          strong  enough,  they  resist  the  motion.  Stability  theory  identifies  a  critical
          Rayleigh  number  above  which  convection  cells  form.   Below  that  Ra,,
          dissipation still damps out motion.
             So let’s explore these two situations by finite element analysis.
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