| タイトル | Distribution of flares on the sun during 1955-1985 - 'Hot spots' (active zones) lasting for 30 years |
| 著者（英） | Bai, Taeil |
| 著者所属（英） | Stanford Univ. |
| 発行日 | 1988-05-15 |
| 言語 | eng |
| 内容記述 | The coordinates of 'major solar flares' observed during the period from January 1955 through August 1985 are analyzed. About 100 'superactive' regions (large, complex, active regions containing large sunspots) produced 46 percent of the major flares during the period. Superactive regions appeared more frequently in certain areas of the sun called 'hot spots' or 'active zones'. The synodic rotation periods of the northern and southern hemisphere hot spots were 26.72 d and 26.61 d, respectively. One of the two hot spots persisted through three solar cycles, and the other was active during cycles 19 and 21 but was dormant during cycle 20. These findings suggest that the mechanism producing hot spots must be stable for two or three solar cycles or longer. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 88A36818 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/370896 |
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