Dynamic stabilization of hydromagnetic surface waves Applications to cometary plasma tails

Details Dynamic stabilization of hydromagnetic surface waves Applications to cometary plasma tails Dynamic stabilization of hydromagnetic surface waves Applications to cometary plasma tails

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...268..420b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 268, May 1, 1983, p. 420-427.

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4

Comet Tails, Magnetohydrodynamic Waves, Solar Wind, Surface Waves, Cosmic Plasma, Dynamic Stability, Electrostatic Waves, Wave Equations, Wave Interaction, Comets, Comet Tails, Plasma, Hydromagnetics, Waves, Fluids, Solar Wind, Electrostatic Effects, Surface, Models, Interaction

Scientific paper

Hydromagnetic waves, at the interface of two superposed magnetofluids, are studied in the presence of electrostatic coherent waves propagating parallel to the surface of discontinuity. Due to nonlinear interaction with the electrostatic waves, hydromagnetic waves, which may be unstable otherwise, can be stabilized. The model developed is applied to study the interaction of the solar wind with the cometary plasma tails.

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