| タイトル | The magnetic field of solar prominences |
| 著者（英） | Klimchuk, J. A.; Antiochos, S. K.; Dahlburg, R. B. |
| 著者所属（英） | NASA Headquarters |
| 発行日 | 1994-01-01 |
| 言語 | eng |
| 内容記述 | A model is presented which accounts for the formation of coronal magnetic field lines with the appropriate 'dipped' structure to support prominences. The critical ingredients of the model are that the prominence magnetic field is a truly three-dimensional structure with significant variation along the prominence length, and the magnetic field is strongly sheared near the photospheric neutral line. Numerical calculations are presented which demonstrate that these two features lead to dip formation. In addition our model is able to account for the long-puzzling observation of inverse polarity in quiescent prominences. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 95A69553 |
| 権利 | Copyright |
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