Thermal anisotropies in the solar wind: Evidence of heating by interstellar pickup ions?
- 1 November 1996
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 23 (22) , 3259-3262
- https://doi.org/10.1029/96gl02909
Abstract
No abstract availableThis publication has 11 references indexed in Scilit:
- Field/field spatial correlation function: Electromagnetic proton cyclotron instabilityJournal of Geophysical Research, 1996
- Heating of the solar wind by pickup ion driven Alfvén ion cyclotron instabilityGeophysical Research Letters, 1996
- Radial evolution of the solar wind from IMP 8 to Voyager 2Geophysical Research Letters, 1995
- Pickup protons and pressure‐balanced structures: Voyager 2 observations in merged interaction regions near 35 AUJournal of Geophysical Research, 1994
- Solar wind velocity and temperature in the outer heliosphereJournal of Geophysical Research, 1994
- Hydromagnetic wave excitation by ionized interstellar hydrogen and helium in the solar windJournal of Geophysical Research, 1987
- The plasma experiment on the 1977 Voyager MissionSpace Science Reviews, 1977
- Interaction of the solar wind with the neutral component of the interstellar gasJournal of Geophysical Research, 1972
- Solar wind proton properties: Vela 3 observations from July 1965 to June 1967Journal of Geophysical Research, 1970
- The Boltzmann equation an d the one-fluid hydromagnetic equations in the absence of particle collisionsProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1956