Computer Science – Sound
Scientific paper
Jan 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993p%26ss...41...21r&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 41, no. 1, p. 21-26.
Computer Science
Sound
26
Magnetohydrodynamic Waves, Plasma Diffusion, Plasma-Electromagnetic Interaction, Space Plasmas, Cosmic Dust, Shock Fronts, Sound Waves, Wave Propagation
Scientific paper
Hydromagnetic waves and shocks in a magnetized three-component dusty plasma are investigated. Dispersion relations for low-frequency modes such as Alfven waves and magnetosonic waves are obtained. Wave-plateau shocks of magnetosonic waves driven by either the upper-hybrid waves or the O-mode electromagnetic waves are shown to exist in a dusty plasma. The shocks allow a transition in the dust flow velocity from submagnetosonic to supermagnetosonic values. Relevance of this transition to simulation results on the interaction of a streaming plasma with a dust cloud is pointed out.
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