A self-consistent model for the particles and fields upstream of an outgassing comet: 2. A time-dependent description
- 1 January 1992
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 97 (A6) , 8173
- https://doi.org/10.1029/92ja00145
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- A self‐consistent model for the particles and fields upstream of an outgassing comet: 1. Gyrotropic and isotropic ion distributionsJournal of Geophysical Research, 1991
- Bulk properties and velocity distributions of water group ions at comet Halley: Giotto measurementsJournal of Geophysical Research, 1990
- Computer simulations of two‐pickup‐ion instabilities in a cometary environmentJournal of Geophysical Research, 1988
- Time scales for formation and spreading of velocity shells of pickup ions in the solar windJournal of Geophysical Research, 1988
- Electron impact ionization in the vicinity of cometsJournal of Geophysical Research, 1987
- A new model of cometary ionospheresJournal of Geophysical Research, 1987
- The development of shell‐like distributions from newborn cometary ionsGeophysical Research Letters, 1986
- Solar wind stagnation near cometsThe Astrophysical Journal, 1985
- Voyager observations of solar wind proton temperature: 1‐10AUGeophysical Research Letters, 1982
- The guiding center approximation to charged particle motionAnnals of Physics, 1961