## Dynamics of convection with magnetic fields |

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5080 channel-attached workstation anelastic approximation bottom boundary boundary conditions buoyancy chaotic behavior continuity equation contours convection cells convection patterns convection with magnetic Cornell National Supercomputer Cornell Theory Center Cornell University density perturbation diffusion parameters downdraft Dynamic behavior Dynamics of Convection field strength Figure 13 Figure 9 finite-difference First-order fixed flow field flux emergence FMAX gauss Ginet and Sudan Glatzmaier global conservation grid horizontal average horizontal magnetic field IBM 5080 channel-attached IBM supercomputing initial conditions kinematic Laboratory of Plasma Lantz 13 length scales magnetic diffusivity magnetic field lines magnetic flux magnetic pressure magnetic tension magneto-anelastic equations magneto-anelastic model magnetoconvection magnetohydrodynamics midpoint parameters momentum equation National Supercomputer Facility nondimensional Nusselt number o.oo partial differential equations passive advection peak physical physical units Plasma Studies pressure PSKX.Z PSl(X.Z regime solar convection zone streamlines strong magnetic fields SUMO code SUMO NRUN Sun's surface fields turbulence two-roll vector