Modeling of pickup ion distributions in the Halley cometosheath: Empirical limits on rates of ionization, diffusion, loss and creation of fast neutral atoms

Author:

Huddleston D. E.,Neugebauer M.,Goldstein B. E.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference38 articles.

1. The ion population between 1300 km and 230 000 km in the coma of comet P/Halley;Altwegg;Astron. Astrophys.,1993

2. Negative ions in the coma of comet Halley;Chaizy;Nature,1991

3. Bulk properties and velocity distributions of water group ions at comet Halley: Giotto measurements;Coates;J. Geophys. Res.,1990

4. The CO and N2 abundance in comet P/Halley;Eberhardt;Astron. Astrophys.,1987

5. Energetic ion fluxes in the inner coma of comet P/Halley;Eviatar;Astrophys. J.,1989

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2. Hybrid code simulations of the solar wind interaction with Comet 19P/Borrelly;Journal of Geophysical Research;2006-12-22

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4. Charge exchange in the solar wind-comet interaction;Journal of Geophysical Research: Space Physics;1997-02-01

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