Particle fluxes observed in the magnetic pileup regions of comets Halley and Grigg-Skjellerup

Details Particle fluxes observed in the magnetic pileup regions of comets Halley and Grigg-Skjellerup Particle fluxes observed in the magnetic pileup regions of comets Halley and Grigg-Skjellerup

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995adspr..16...29k&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 16, no. 4, p. (4)29-(4)34

Physics

2

Energetic Particles, Flux (Rate), Grigg-Skjellerup Comet, Halley'S Comet, Interplanetary Magnetic Fields, Ions, Particle Acceleration, Cavities, Cometary Magnetospheres, Giotto Mission, Particle Telescopes, Vega Project

Scientific paper

Energetic particles (EH2O greater than or equal to 60 keV) as well as plasma ions of a few KeV in energy have been measured in the magnetic pileup region and in the cavity of comet Halley (13/14 March 1986) by the instruments EPA/EPONA, RPA and IMS. The Pileup region of comet Grigg-Skjellerup (G-S) was traversed on 10 July 1992. Similarities and diversities in the encounter conditions, particle fluxes and acceleration processes at both comets are discussed.

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