Solar-wind instability near bodies

Details Solar-wind instability near bodies Solar-wind instability near bodies

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24..705v&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, Sept.-Oct. 1984, p. 705-708. In Russian.

Physics

Flow Stability, Magnetohydrodynamic Flow, Solar Wind, Deceleration, Hydrodynamic Equations, Shear Properties, Velocity Distribution, Viscosity

Scientific paper

The hydrodynamic instability of waves in the solar wind near planets and comets is examined theoretically. It is shown that this instability is caused by the nonuniformity of the velocity field, i.e., flow deceleration and shear. The increment of local instability is determined; the instability characteristics at points in front of and behind the body are analyzed; and the effect of viscosity is investigated.

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