| タイトル | Application of the MHD energy principle to magnetostatic atmospheres |
| 本文（外部サイト） | http://hdl.handle.net/2060/19850021108 |
| 著者（英） | Zweibel, E. G. |
| 著者所属（英） | Colorado Univ. |
| 発行日 | 1984-01-01 |
| 言語 | eng |
| 内容記述 | The MHD energy principle is applied to the stability of a magnetized atmosphere which is bounded below by much denser fluid, as is the solar corona. The two fluids are treated as ideal; the approximation is consistent with the energy principle, and the dynamical conditions that must hold at a fluid-fluid interface are used to show that if vertical displacements of the lower boundary are premitted, then the lower atmosphere must be perturbed as well. However, displacements which do not perturb the coronal boundary can be properly treated as isolated perturbations of the corona alone. |
| NASA分類 | GEOPHYSICS |
| レポートNO | 85N29420
NASA-CR-175967
NAS 1.26:175967 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/156163 |
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