Position and structure of the shock wave in the vicinity of Comet Halley according to VEGA 1 and 2 measurements

Details Position and structure of the shock wave in the vicinity of Comet Halley according to VEGA 1 and 2 measurements Position and structure of the shock wave in the vicinity of Comet Halley according to VEGA 1 and 2 measurements

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kosis..25..900g&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 25, Nov.-Dec. 1987, p. 900-906. In Russian.

Physics

Halley'S Comet, Plasma Interactions, Shock Waves, Solar Wind, Spaceborne Experiments, Vega Project, Energy Distribution, Plasma Turbulence

Scientific paper

Vega 1 and 2 measurements indicated the presence of strong MHD turbulence in the vicinity of Comet Halley. The cometocentric-distance dependence of the solar-wind parameters in the vicinity of the near-cometary shock wave is examined for various positions of the Vega probes in relation to the comet. In addition, the oscillation spectra of electric and magnetic fields of plasma waves in the vicinity of the near-cometary shock front are analyzed.

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