Influence of non-Bi-Maxwellian distribution function of solar wind protons on the ion cyclotron instability-Reference-Cited by-同舟云学术

Influence of non-Bi-Maxwellian distribution function of solar wind protons on the ion cyclotron instability

Published:1978 Issue:A8 Volume:83 Page:3900
ISSN:0148-0227
Container-title:Journal of Geophysical Research
language:en
Short-container-title:J. Geophys. Res.

Author:

Leubner M. P.

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

Link

http://www.agu.org/journals/ja/v083/iA08/JA083iA08p03900/JA083iA08p03900.pdf

Reference14 articles.

1. Electromagnetic ion-cyclotron wave growth rates and their variation with velocity distribution function shape;Abraham-Shrauner;J. Plasma Phys.,1977

2. Cap, F. F., , Handbook on Plasma Instabilities, , 1, Academic, New York, 1976,

3. On the origin of solar wind proton thermal anisotropy;Feldman;J. Geophys. Res.,1973

4. Empirical closure relation for the Vlasov moment equations;Feldman;Phys. Rev. Lett.,1973

5. Double ion streams in the solar wind;Feldman;J. Geophys. Res.,1973

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