A new axisymmetric MHD model of the interaction of the solar wind with Venus-Reference-Cited by-同舟云学术

A new axisymmetric MHD model of the interaction of the solar wind with Venus

Published:1996-02-01 Issue:E2 Volume:101 Page:4547-4556
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res.

Author:

De Zeeuw Darren L.,Nagy Andrew F.,Gombosi Tamas I.,Powell Kenneth G.,Luhmann Janet G.

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/je/v101/iE02/95JE03363/95JE03363.pdf

Reference25 articles.

1. Interplanetary field control of the location of the Venus bow shock: Evidence for comet-like ion pickup;Alexander;Geophys. Res. Lett.,1986

2. The effect of hot oxygen corona on the interaction of the solar wind with Venus;Belotserkovskii;Geophys. Res. Lett.,1987

3. Magnetic asymmetries of unmagnetized planets;Brecht;Geophys. Res. Lett.,1990

4. Global hybrid simulation of unmagnetized planets: Comparison of Venus and Mars;Brecht;J. Geophys. Res.,1991

5. Three-dimensional simulation of the solar wind interaction with Mars;Brecht;J. Geophys. Res.,1993

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