| タイトル | Development of a computational model for predicting solar wind flows past nonmagnetic terrestrial planets |
| 本文（外部サイト） | http://hdl.handle.net/2060/19830028774 |
| 著者（英） | Spreiter, J. R.; Stahara, S. S. |
| 著者所属（英） | Nielsen Engineering and Research, Inc. |
| 発行日 | 1983-10-01 |
| 言語 | eng |
| 内容記述 | A computational model for the determination of the detailed plasma and magnetic field properties of the global interaction of the solar wind with nonmagnetic terrestrial planetary obstacles is described. The theoretical method is based on an established single fluid, steady, dissipationless, magnetohydrodynamic continuum model, and is appropriate for the calculation of supersonic, super-Alfvenic solar wind flow past terrestrial ionospheres. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 83N37045
NEAR-TR-313
NASA-CR-174455
NAS 1.26:174455 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/161299 |
