| タイトル | Studies of Solar Wind Interaction and Ionospheric Processes at Venus and Mars |
| 本文（外部サイト） | http://hdl.handle.net/2060/20030052280 |
| 著者（英） | Nagy, Andrew F.; Bogan, Denis |
| 著者所属（英） | Michigan Univ. |
| 発行日 | 2003-05-14 |
| 言語 | eng |
| 内容記述 | This is the final report summarizing the work done during the last three years under NASA Grant NAG5-8946. Our efforts centered on a systematic development of a new generation of three dimensional magneto-hydrodynamic (MHD) numerical code, which models the interaction processes of the solar wind or fast flowing magnetospheric plasma with 'non-magnetic' solar system bodies (e.g. Venus, Mars, Europa, Titan). We have also worked on a number of different, more specific and discrete studies, as various opportunities arose. In the next few pages we briefly summarize these efforts. |
| NASA分類 | Lunar and Planetary Science and Exploration |
| レポートNO | UM-F002579/039577 |
| 権利 | No Copyright |
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