| タイトル | Dynamic formation and magnetic support of loop or arcade prominences |
| 著者（英） | Vanhoven, Gerard; Mok, Y.; Drake, J. F. |
| 著者所属（英） | California Univ. |
| 発行日 | 1992-11-01 |
| 言語 | eng |
| 内容記述 | The results of model dynamic simulations of the formation and support of a narrow prominence at the apex of a coronal magnetic loop or arcade are described. The condensation process proceeds via an initial radiative cooling and pressure drop, and a secondary siphon flow from the dense chromospheric ends. The antibuoyancy effect as the prominence forms causes a bending of a confining magnetic field, which propagates toward the semirigid ends of the magnetic loop. Thus, a wide magnetic 'hammock' or well (of a normal polarity Kippenhahn-Schlueter type) is formed, which supports the prominence at or near the field apex. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 93N31391 |
| 権利 | Copyright, Distribution within the U.S. granted by agreement |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/230111 |
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