Effects on the Jovian magnetosheath arising from solar wind flow around nonaxisymmetric bodies-Reference-Cited by-同舟云学术

Effects on the Jovian magnetosheath arising from solar wind flow around nonaxisymmetric bodies

Published:1996-05-01 Issue:A5 Volume:101 Page:10665-10672
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res.

Author:

Erkaev N. V.,Farrugia C. J.,Biernat H. K.

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/v101/iA05/95JA03518/95JA03518.pdf

Reference14 articles.

1. Magnetosheath parameters and reconnection' A case study for the near-cusp region and the equatorial flank;Biernat;Planet. Space Sci.,1995

2. Idealized Jovian magnetosphere shape and field;Engle;J. Geophys. Res.,1980

3. The results of study of MHD flow around magnetosphere (in Russian);Erkaev;Geomagn. Aeron.,1988

4. The solar wind flow along the subsolar line in the magnetic barrier and reconnection at the magnetopause;Erkaev;Adv. Space Res.,1994

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