| タイトル | Rapid changes in the fine structure of a coronal 'bright point' and a small coronal 'active region' |
| 著者（英） | Sheeley, N. R., Jr.; Golub, L. |
| 著者所属（英） | Harvard-Smithsonian Center for Astrophysics|Hulburt (E. O.) Center for Space Research |
| 発行日 | 1979-08-01 |
| 言語 | eng |
| 内容記述 | A coronal bright point is resolved into a pattern of emission which, at any given time, consists of 2 or 3 miniature loops (each approximately 2500 km in diameter and approximately 2000 km long). During the half-day lifetime of the 'bright point' individual loops evolved on a time scale approximately 7 min. A small 'active region' seemed to evolve in this way, but the occasional blurring together of several loops made it difficult to follow individual changes. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 79A51588 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/425422 |
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