The region of cometary ions in the head of Comet Halley according to Vega-2 data

Details The region of cometary ions in the head of Comet Halley according to Vega-2 data The region of cometary ions in the head of Comet Halley according to Vega-2 data

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kosis..25..914g&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 25, Nov.-Dec. 1987, p. 914-920. In Russian.

Astronomy and Astrophysics

Astronomy

Comet Heads, Halley'S Comet, Heavy Ions, Plasma Diagnostics, Vega Project, Astronomical Spectroscopy, Plasma Interactions, Solar Wind

Scientific paper

Vega Plazmag-1 measurements revealed the existence of a cometopause about 160,00 km from the nucleus of Comet Halley. This cometopause divides the external region (controlled by solar-wind protons) from the internal region of the cometary plasma, where heavy cometary ions predominate. This paper presents additional experimental data, and examines the physical characteristics of the cometary-plasma region.

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