| タイトル | The solar wind mass flux |
| 著者（英） | Withbroe, George L. |
| 著者所属（英） | Harvard-Smithsonian Center for Astrophysics |
| 発行日 | 1989-02-01 |
| 言語 | eng |
| 内容記述 | One of the unexplained observations of the solar wind at 1 AU is the relative constancy of the solar wind mass flux. Calculations using a radiative energy balance model with a thermally driven wind suggest that this near constancy of the mass (particle) flux is due to two factors: (1) the role of inward conduction and radiation in cooling the corona, and (2) the finding that the particle flux is proportional to the gas pressure in the outer corona and beyond, where the solar wind flow becomes radial. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 89A26929 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/365302 |
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