The Physics of Fluids · 1966 · 418 citations · 5 references
Natural SciencesPhysicsElectromagnetismFluid DynamicsPlasma PhysicsMagnetized PlasmaPlasma InstabilitiesPlasma WavesAlfven WavesAlfvén WavesCollisionless DissipationCollisionless Plasma DynamicsElectron HeatingIon HeatingMode DampingStatic Magnetic Field
Except for the Alfvén (shear) mode, all hydromagnetic waves are strongly damped in plasmas of moderate or high β (fluid pressure/magnetic pressure). The study also examines the modes associated with the hose and mirror plasma instabilities in detail. Numerical solutions of the dispersion relation reveal that for β>½ the fast mode is damped a few percent more than the slow mode (≈½), and the fast magnetosonic mode displays two damping maxima—one at 20°–40° associated with ion heating and another at 85°–89° associated with electron heating.
Numerical solutions have been obtained for the dispersion relation for hydromagnetic waves in an infinite, uniform, collisionless plasma. Except for the Alfvén (shear) mode, all hydromagnetic waves are strongly damped in plasmas of moderate or high β (fluid pressure/magnetic pressure). For β greater than about ½, the damping factor W=−Im (ω)/|Re (ω)| is a few percent greater for the fast mode (except for special directions of propagation) and of order ½ for the slow mode. The least damped (fast) magnetosonic mode exhibits two maxima in a plot of W versus the angle θ between the wave vector k and the static magnetic field: the first maximum occurs for θ between 20° and 40° and is associated with ion heating; the second occurs between 85° and 89° and is associated with electron heating. In addition, the modes associated with the ``hose'' and ``mirror'' plasma instabilities are considered in some detail.
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<i>Hydrodynamic and Hydromagnetic Stability</i>
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William B. Thompson, W. T. Payne · American Journal of Physics · 1964 · 209 citations · Full text