| タイトル | The 3-D solar radioastronomy and the structure of the corona and the solar wind |
| 本文（外部サイト） | http://hdl.handle.net/2060/19760017036 |
| 著者（英） | Steinberg, J. L.; Caroubalos, C. |
| 著者所属（英） | Observatoire de Paris-Meudon |
| 発行日 | 1976-03-01 |
| 言語 | eng |
| 内容記述 | The mechanism causing solar radio bursts (1 and 111) is examined. It is proposed that a nonthermal energy source is responsible for the bursts; nonthermal energy is converted into electromagnetic energy. The advantages are examined for an out-of-the-ecliptic solar probe mission, which is proposed as a means of stereoscopically viewing solar radio bursts, solar magnetic fields, coronal structure, and the solar wind. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 76N24124 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/569863 |
