Two sympathetic homologous CMEs on 2002 May 22

被引:19
作者
Cheng, JX [1 ]
Fang, C [1 ]
Chen, PF [1 ]
Ding, MD [1 ]
机构
[1] Nanjing Univ, Dept Astron, Nanjing 210093, Peoples R China
来源
CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS | 2005年 / 5卷 / 03期
关键词
sun : filament; sun : flares; sun : CMEs;
D O I
10.1088/1009-9271/5/3/006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Sympathetic coronal mass ejections (CMEs) usually occur in different active regions connected by interconnecting magnetic loops, while homologous CMEs occur within the same active region with an almost the same background magnetic field, and so are similar in shapes. Two sympathetic CMEs erupted within 3 hours on 2002 May 22, originating from the same active region, AR 9948. Their multi-wavelength data were collected and analyzed. It is suggested that emerging flux triggered the occurrence of the first CME and the corresponding flare, the reconnection inflow of which in turn triggered the eruption of the second CME. Based on the fact that the two sympathetic CMEs, have many similarities, in their shapes, their low-lying dimming areas, etc., we tentatively propose, for the first time, the phenomenon of sympathetic homologous CMEs.
引用
收藏
页码:265 / 272
页数:8
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