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Plasma in a Magnetic Field
The Interaction of a Magnetic Field and
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acceleration active regions adiabatic Alfven wave amplitude approximation astrophysics average causes chromosphere collisions component compression Consequently constant convection corona cosmic electrodynamics cosmic rays curl damping decreases density depends determined direction displacement dissipation distance disturbance earth effect electric field equal to zero equation equilibrium faculae flares flow flux frequency front galaxy gravitational greater heat homogeneous hydrodynamic increase inhomogeneous instability intensity ionized gas ionosphere ions and electrons isotropic Joule losses kilometers layers lines of force liquid magnetic energy magnetic field magnetic forces magnetohydrodynamic mean free path medium motion moving nebula observed obtain oersteds Ohm's law oscillations parsecs particles perpendicular photosphere Pikel'ner plane plasma waves polar presence prominences propagated pulsations quantity radiation radio radius random reference result rotation scale shock wave stability stars steady-state sunspots surface takes place temperature thermal conductivity tion toroidal field turbulence vector velocity virial theorem viscosity zone