Support for the shock source hypothesis of upstream whistlers from hall-MHD calculations-Reference-Cited by-同舟云学术

Support for the shock source hypothesis of upstream whistlers from hall-MHD calculations

Published:1995-01 Issue:8-9 Volume:15 Page:93-96
ISSN:0273-1177
Container-title:Advances in Space Research
language:en
Short-container-title:Advances in Space Research

Author:

Baumgärtel K,Sauer K

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference8 articles.

1. D.S.Orlowski, C.T. Russell, D. Kraus-Varban, and N. Omidi, On the source of upstream whistlers in the Venus foreshock, in: Plasma environments of non-maggnetic planets, Proc. 4th COSPAR Colloquium, Ann Arbor, Michigan, ed. T.I. Gombosi, p. 217, 19932.

2. Whistler waves observed upstream from collisionless shocks;Fairfield;J. Geophys. Res.,1974

3. Bow shock and magnetosheath waves at Mercury;Fairfield;J. Geophys. Res.,1976

4. Upstream waves at Mercury, Venus and Earth: Comparison of the properties of one Hertz waves;Orlowski;Geophys. Res. Lett.,1990

5. ULF waves upstream uf the Venus bow shock: properties of one-Hertz waves;Orlowski;J. Geophys. Res.,1991

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4. Observations of low-frequency electromagnetic plasma waves upstream from the Martian shock;Journal of Geophysical Research;2002