Influence of instabilities on plasma flow around a comet

Details Influence of instabilities on plasma flow around a comet Influence of instabilities on plasma flow around a comet

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jgr....94...15k&link_type=abstract

(Chapman Conference on Plasma Waves and Instabilities in Magnetospheres and at Comets, Sendai, Japan, Oct. 12-16, 1987) Journal

Other

11

Comet Tails, Magnetohydrodynamic Flow, Magnetohydrodynamic Stability, Oxygen Ions, Space Plasmas, Drift Rate, Ion Motion, Solar Wind, Comets, Stability, Plasma, Flows, Ions, Motion, Solar Wind, Fluids, Magnetohydrodynamics, Calculations, Diagrams, Comet Tails, Velocity

Scientific paper

A multifluid hydrodynamic approximation allowing for the relative motion along the magnetic field of the newly created ions and the original fluid is used to treat the ion-pickup process. Due to the processes characterized by these means, the ion tail of a comet may not be antisolar; the derivation from radial is anticipated to be largest for oxygen due to its ionization at the greatest distances. Other ions, created nearer the comet where flow speed is lower, should have smaller transverse velocities.

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