The filament disappearance of 7 May 1992 (the EBI)

被引:11
作者
Mouradian, Z [1 ]
Soru-Escaut, I
Hiei, E
McAllister, AH
Shibasaki, K
Ohyama, M
Khan, JI
Uchida, Y
机构
[1] Observ Paris, F-92195 Meudon, France
[2] Iwaki Meisei Univ, Hino, Tokyo 191, Japan
[3] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80307 USA
[4] Nobeyama Radio Observ, Minamisa Ku, Nagano 38413, Japan
[5] Natl Astron Observ, Mitaka, Tokyo 181, Japan
[6] UCL, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[7] Tokyo Univ Sci, Dept Phys, Shinjuku Ku, Tokyo 162, Japan
关键词
Flare; Active Region; Velocity Phase; General Effect; Main Body;
D O I
10.1023/A:1005079225096
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The 7 May 1992 filament disappearance in the low corona is analyzed. The cool and hot components of this event are studied, using H alpha, soft X-ray and radio data. We first show the general effect of the disparition brusque (DB) on the life of the filament, which was a quiescent filament in the vicinity of an active region, and then give the history of the development of the 7 May event. The main stages of the event are: (i) the formation of hot arches spanning the cool filament; (ii) rise of the filament, with plasma ejection into the corona, in which we note some spreading of loops from the main body, with two distinct rising velocity phases of the H alpha filament; (iii) formation of X-ray arches below the filament, the foot points of the arcades being two-ribbon H alpha hare patches. The dynamics of H alpha and X-rays features are given.
引用
收藏
页码:313 / 329
页数:17
相关论文
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