The electron density and temperature in the tail of Comet Giacobini-Zinner

Details The electron density and temperature in the tail of Comet Giacobini-Zinner The electron density and temperature in the tail of Comet Giacobini-Zinner

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986georl..13..405m&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 13, April 1986, p. 405, 406.

Physics

9

Comet Tails, Electron Density (Concentration), Giacobini-Zinner Comet, Atmospheric Models, Electron Energy, Water Vapor, Comets, Giacobini-Zinner, Electrons, Density, Temperature, Comet Tails, Calculations, Models, Water, Atmosphere, Ice Mission, Comparisons, Spacecraft Observations, Plasma Electron Experiment

Scientific paper

The electron density and temperature profiles along the tail axis of comet Giacobini-Zinner are calculated, using a multifluid model of an H2O-dominated atmosphere. The results obtained using this model, which was developed prior to ICE, are compared to the data from the mission and are found to be in satisfactory agreement with the ICE observations.

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