| タイトル | The stability of coronal and prominence magnetic fields |
| 本文（外部サイト） | http://hdl.handle.net/2060/19870011508 |
| 著者（英） | Hood, A. W. |
| 著者所属（英） | Saint Andrew's Univ. |
| 発行日 | 1986-12-01 |
| 言語 | eng |
| 内容記述 | The significance of the localized instabilities is not yet fully understood. The nonlinear coupling of these modes may give rise to an explosive instability, with the modes coupling to longer wavelengths. On the other hand, if the modes saturate early, than the main effect of the instability may be an enhancement of transport coefficients. Nonetheless, the equation provides a simple test for the stability of cylindrical magnetic fields. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 87N20941 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/151096 |
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