Super-active regions in solar cycle 24

被引:9
|
作者
Chen, Anqin [1 ,2 ]
Wang, Jingxiu [2 ]
机构
[1] China Meteorol Adm, Natl Ctr Space Weather, Key Lab Space Weather, Beijing 100081, Peoples R China
[2] Chinese Acad Sci, Key Lab Solar Act, Natl Astron Observ, Beijing 100012, Peoples R China
来源
基金
中国国家自然科学基金;
关键词
Sun: activity; Sun: magnetic field; Sun: active regions;
D O I
10.1017/S1743921316000223
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Comparing with solar cycles 21-23, the level of solar activity in the current cycle is very low. So far, there have been only five SARs and 45 X class flares. The monthly smoothed total solar irradiance decreased sharply by 0.09% from the maximum of cycle 23 to the minima between cycles 23 and 24. In this contribution, we present new studies on SARs in Cycle 24. The SARs in the current cycle have relatively smaller flare index (ifi) and composite vector field index () comparing with the SARs in cycles 22 and 23. There is a clearly linear relationship between and The emphasis of this contribution is put on the similarity and different behaviors of vector magnetic fields of the SARs in the current solar cycle and the previous ones. We try to get a satisfactory account for the general characteristics and relatively lower level of solar flare activity in Cycle 24.
引用
收藏
页码:309 / 314
页数:6
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