Generation of solar wind proton tails and double beams by Coulomb collisions
- 1 July 1987
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 92 (A7), 7255-7261
- https://doi.org/10.1029/ja092ia07p07255
Abstract
No abstract availableKeywords
This publication has 17 references indexed in Scilit:
- Modern exospheric theories and their observational relevanceReviews of Geophysics, 1983
- Electromagnetic kinetic instabilities in multicomponent space plasmas: Theoretical predictions and computer simulation experimentsReviews of Geophysics, 1981
- Ion acoustic waves and related plasma observations in the solar windJournal of Geophysical Research, 1979
- Suprathermal protons in the interplanetary solar windJournal of Geophysical Research, 1976
- Interpenetrating solar wind streamsReviews of Geophysics, 1974
- On the origin of solar wind proton thermal anisotropyJournal of Geophysical Research, 1973
- Double ion streams in the solar windJournal of Geophysical Research, 1973
- The anisotropy of the solar windPlanetary and Space Science, 1969
- Electron and Ion Runaway in a Fully Ionized Gas. IIPhysical Review B, 1960
- A Model for Collision Processes in Gases. I. Small Amplitude Processes in Charged and Neutral One-Component SystemsPhysical Review B, 1954