Physics
Scientific paper
Jul 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phflb...3.1728b&link_type=abstract
Physics of Fluids B (ISSN 0899-8221), vol. 3, July 1991, p. 1728-1738.
Physics
23
Ampte (Satellites), Barium Ion Clouds, Magnetohydrodynamic Stability, Plasma Clouds, Solar Wind, Magnetohydrodynamic Turbulence, Plasma-Particle Interactions, Solar Protons
Scientific paper
The neutral Ba atoms released in the solar wind by the AMPTE mission satellite underwent rapid photoionization, forming a dense, expanding plasma cloud which interrupted the solar wind flow, giving rise to diamagnetic cavities; on their upstream side, a region of compressed plasma and enhanced magnetic field was created due to the deceleration and deflection of the solar wind and magnetic field-line draping. Attention is presently given to the ways in which the newly created expanding plasma couples to the solar wind, by means of plasma-beam and current-driven instabilities. It is shown how lower-hybrid and lower-hybrid drift waves are generated by cross-field proton-barium streaming instabilities and cross-field electron currents.
Bingham Richard
de Angelis Umberto
Gil'Man M.
Shapiro Vitali D.
Tsytovich Vadim N.
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