| タイトル | The Faraday rotation experiment |
| 著者（英） | Volland, H.; Levy, G. S.; Seidel, B. L.; Bird, M. K.; Stelzried, C. T. |
| 著者所属（英） | Bonn Univ.; Jet Propulsion Lab., California Inst. of Tech. |
| 発行日 | 1984-01-01 |
| 言語 | German
eng |
| 内容記述 | The magnetized plasma of the solar corona was remotely sounded using the Faraday rotation effect. The solar magnetic field together with the electrons of the coronal plasma cause a measurable Faraday rotation effect, since the radio waves of Helios are linearly polarized. The measurement is performed at the ground stations. Alfven waves traveling from the Sun's surface through the corona into interplanetary space are observed. Helios 2 signals penetrating through a region where coronal mass is ejected show wavelike structures. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 85N27805 |
| 権利 | No Copyright |
|
