Time evolution of a two-ribbon flare - Characteristics of post-flare loops | |
Gu XM(顾啸马)1; Lin J(林隽)1; Luan D(栾蒂)1; SCHMIEDER, B2 | |
发表期刊 | ASTRONOMY & ASTROPHYSICS |
1992-06 | |
卷号 | 259期号:2页码:649-662 |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Corona Sun Flares |
摘要 | Observations of a two ribbon flare on 5 May, 1989 were performed at Yunnan Observatory and at Meudon. Magnetograms have been obtained in Huairou-Beijing Observatory. The topology of the flaring region and the slow evolution of post-flare loops (cool flare loops) can be derived from Yunnan filtergrams. The ribbons seem to be the footpoints of the loops. The analysis of Ha line profiles in the loops, obtained with the Multichannel Subtractive Double Pass (MSDP) spectrograph of Meudon allows us to derive some physical parameters of the loops. The importance of the reference background intensity is discussed. The cool flare loops are low (h(max) approximately 25000km) dense (ne approximately 10(11) cm-3) and relatively inhomogeneous. They are rising with a velocity of 5 to 10 km s-1. |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 0004-6361 |
URL | 查看原文 |
WOS记录号 | WOS:A1992JB31800041 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | H-ALPHA ; GRADUAL PHASE ; SOLAR-FLARES ; EVAPORATION |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/6007 |
专题 | 太阳物理研究组 |
作者单位 | 1.Yunnan Observatory, Academica Sinica, P.O.Box 110, Kunming, People's Republic of China 2.DASOP, Observatoire de Paris, Section de Meudon, F-92195 Meudon Principal Cedex, France |
第一作者单位 | 中国科学院云南天文台 |
推荐引用方式 GB/T 7714 | Gu XM,Lin J,Luan D,et al. Time evolution of a two-ribbon flare - Characteristics of post-flare loops[J]. ASTRONOMY & ASTROPHYSICS,1992,259(2):649-662. |
APA | Gu XM,Lin J,Luan D,&SCHMIEDER, B.(1992).Time evolution of a two-ribbon flare - Characteristics of post-flare loops.ASTRONOMY & ASTROPHYSICS,259(2),649-662. |
MLA | Gu XM,et al."Time evolution of a two-ribbon flare - Characteristics of post-flare loops".ASTRONOMY & ASTROPHYSICS 259.2(1992):649-662. |
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