Physical Review Letters · 1994 · 57 citations · 26 references
Natural SciencesPhysicsComputational PhysicsFluid DynamicsPlasma PhysicsMagnetized PlasmaMagnetohydrodynamicsNonlinear Plasma DynamicsPlasma InstabilitiesPlasma SimulationVortex DynamicsHall EffectHall MagnetohydrodynamicsKelvin-helmholtz InstabilityMagnetohydrodynamic InstabilitiesMagnetohydrodynamic SimulationsNonlinear EvolutionNonlinear SystemsVortex Formation
The nonlinear evolution of the Kelvin-Helmholtz instability in an inhomogeneous plasma is studied using a two-dimensional magnetohydrodynamic (MHD) simulation code which includes the Hall term. This term is important when the thickness of the boundary layer is less than an ion inertial length. In comparison to the evolution of the instability based upon ideal MHD, the Hall term generates short wavelength turbulence which inhibits vortex formation, and introduces an asymmetry into the nonlinear evolution of the instability depending upon the sign of the vorticity.
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