Three-dimensional MHD simulation of the solar wind interaction with the ionosphere of Venus: Results of two-component reacting plasma simulation

Author:

Tanaka T.,Murawski 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

Reference47 articles.

1. The structure of the Venus ionosphere;Brace;Space Sci. Rev.,1991

2. The nightward ion flow scenario at Venus revisited;Brace;Adv. Space Res.,1995

3. Three dimensional MHD simulations of the interaction between Venus and the solar wind;Cable;J. Geophys. Res.,1995

4. Steady state flow/field model of solar wind interaction with Venus: Global implications of local effects;Cloutier;J. Geophys. Res.,1987

5. The ionospheric peak on the Venus dayside;Cravens;J. Geophys. Res.,1981

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