A three-dimensional, multispecies, comprehensive MHD model of the solar wind interaction with the planet Venus-Reference-Cited by-同舟云学术

A three-dimensional, multispecies, comprehensive MHD model of the solar wind interaction with the planet Venus

Published:2009-09 Issue:A9 Volume:114 Page:n/a-n/a
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res.

Author:

Terada N.¹²,Shinagawa H.¹²,Tanaka T.²³,Murawski K.⁴,Terada K.⁵

Affiliation:

1. Space Environment Group, Applied Electromagnetic Research Center; National Institute of Information and Communications Technology; Tokyo Japan

2. Core Research for Evolutional Science and Technology; Japan Science and Technology Agency; Saitama Japan

3. Department of Earth and Planetary Sciences, Faculty of Sciences; Kyushu University; Fukuoka Japan

4. Group of Astrophysics and Gravity Theory; UMCS; Lublin Poland

5. Department of Geophysics, Graduate School of Science; Kyoto University; Kyoto Japan

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

Reference57 articles.

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3. A multiscale central difference scheme applied to magnetohydrodynamic simulations of cometary atmospheres;Benna;Astrophys. J.,2004

4. Modeling the response of the induced magnetosphere of Venus to changing IMF direction using MESSENGER and Venus Express observations;Benna;Geophys. Res. Lett.,2009

5. Photoabsorption and photoionisation measurements on some atmospheric gases in the wavelength region 50-340 A;Cole;J. Phys. B At. Mol. Phys.,1978

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