A NARROW STREAMER-PUFF CORONAL MASS EJECTION FROM THE NONRADIAL ERUPTION OF AN ACTIVE-REGION FILAMENT | |
Jiang YC(姜云春); Yang JY(杨家艳); Zheng RS(郑瑞生); Bi Y(毕以); Yang XL(杨晓林); Jiang, YC (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Astron Observ, POB 110, Kunming 650011, Peoples R China. | |
发表期刊 | ASTROPHYSICAL JOURNAL |
2009-03-10 | |
卷号 | 693期号:2页码:1851-1858 |
DOI | 10.1088/0004-637X/693/2/1851 |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Sun: Activity Sun: Coronal Mass Ejections (Cmes) Sun: Filaments Sun: Flares |
摘要 | So-called streamer-puff coronal mass ejections (CMEs) were recently identified by Bemporad et al. as a new variety of CME. They originate from nonradial ejecta from compact ejective flares occurring in the outskirts of the base of a streamer and travel out along it, during which the streamer is transiently inflated by the puff but is not disrupted. Moore & Sterling further indicated that streamer-puff CMEs are a particular subclass of a broad class of CMEs, called "over-and-out" CMEs, which come from flare-producing magnetic explosions of various sizes and are laterally far offset from the flare. In this paper, we present observations of a streamer-puff CME that resulted from the spectacular eruption of an active-region filament inside a single helmet streamer consisting of a double-arcade system, occurring in AR 10792 on 2005 July 29. The filament was covered by a smaller arcade in the outer flank of the streamer base, with a nearby quiescent prominence below another larger arcade. In the inner corona the filament eruption underwent nonradial motion, while in the outer corona the CME had a radial path along the streamer that was laterally offset from the original site of the filament. The CME was narrow with an angular width of only 15. and clearly showed a typical three-part structure below 1.38 R(circle dot). In this eruption, the prominence remained nearly unchanged, but in other stronger eruptions of a homologous sequence from the same AR in the following days, it exhibited obvious oscillations. These observations can be explained by the magnetic-arch-blowout scenario for streamer-puff and over-and-out CMEs, in which the streamer arcade can act on the erupting filament, laterally deflecting and channeling its motion. The prominence oscillations probably indicate an interplay or interaction between the twin arcades that could affect but not destroy the overall field configuration supporting the prominence. |
项目资助者 | National Center for Atmospheric Research ; National Science Foundation ; Natural Science Foundation of China [10573033, 40636031] ; Scientific Application Foundation of Yunnan Province [2007A112M] |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 0004-637X |
URL | 查看原文 |
归档日期 | 2009-03-12 |
WOS记录号 | WOS:000264095100073 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | LASCO OBSERVATIONS ; SOLAR-ACTIVITY ; PROMINENCE ; FLARES ; SOHO ; CAVITIES ; TRANSIENTS ; EVOLUTION ; CHIRALITY ; DYNAMICS |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/6147 |
专题 | 太阳物理研究组 |
通讯作者 | Jiang, YC (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Astron Observ, POB 110, Kunming 650011, Peoples R China. |
作者单位 | National Astronomical Observatories/Yunnan Astronomical Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming 650011, China |
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 | Jiang YC,Yang JY,Zheng RS,et al. A NARROW STREAMER-PUFF CORONAL MASS EJECTION FROM THE NONRADIAL ERUPTION OF AN ACTIVE-REGION FILAMENT[J]. ASTROPHYSICAL JOURNAL,2009,693(2):1851-1858. |
APA | Jiang YC,Yang JY,Zheng RS,Bi Y,Yang XL,&Jiang, YC .(2009).A NARROW STREAMER-PUFF CORONAL MASS EJECTION FROM THE NONRADIAL ERUPTION OF AN ACTIVE-REGION FILAMENT.ASTROPHYSICAL JOURNAL,693(2),1851-1858. |
MLA | Jiang YC,et al."A NARROW STREAMER-PUFF CORONAL MASS EJECTION FROM THE NONRADIAL ERUPTION OF AN ACTIVE-REGION FILAMENT".ASTROPHYSICAL JOURNAL 693.2(2009):1851-1858. |
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