Vega-probe measurements of plasma waves

Details Vega-probe measurements of plasma waves Vega-probe measurements of plasma waves

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kosis..25..943k&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 25, Nov.-Dec. 1987, p. 943-951. In Russian.

Other

Cometary Atmospheres, Halley'S Comet, Plasma Diagnostics, Plasma Waves, Solar Wind, Vega Project, Ion Production Rates, Satellite-Borne Instruments

Scientific paper

The Vega APV-N experiment for the investigation of low-frequency plasma waves in the vicinity of Comet Halley is described. Results are presented on collective processes in the plasma responsible for the formation of fine structures in the solar wind/cometary atmosphere interaction region and for the dissipation of solar-wind energy in this region. Other aspects of the experiment were: (1) the determination of the anomalous ionization of the cometary atmosphere in the presence of the magnetized solar wind and the identification of ionization mechanisms; and (2) plasma diagnostics in the solar wind and the cometary ionosphere via measurements of characteristic boundaries in the cometary plasma shell.

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