Magnetic flux cancellation associated with the major solar event on 2000 July 14

被引:114
|
作者
Zhang, J
Wang, JX
Deng, YY
Wu, DJ
机构
[1] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
[2] Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
来源
ASTROPHYSICAL JOURNAL | 2001年 / 548卷 / 01期
基金
中国国家自然科学基金;
关键词
Sun : coronal mass ejections (CMEs) Sun : filaments; Sun : flares; Sun : magnetic fields;
D O I
10.1086/318934
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The major solar event on 2000 July 14 is characterized by the simultaneous occurrence of a giant filament eruption, a great flare, and an extended Earth-directed coronal mass ejection. We examined in detail the magnetic evolution in its source active region, NOAA 9077, and found that the only obvious magnetic change in the course of the event is magnetic flux cancellation at many sites in the vicinity of the filament. Moreover, all the initial disturbance in the filament and the initial brightening around the filament took place at the cancellation sites. It is clearly indicated that the slow magnetic reconnection in the lower atmosphere, which is manifested as observed flux cancellation, is of overwhelming importance in leading to the global instability responsible for the major magnetic activity.
引用
收藏
页码:L99 / L102
页数:4
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