The coronal mass ejection associated with the loop eruption and coronal dimmings on 2009 December 13 | |
Zheng RS(郑瑞生)1,2![]() ![]() ![]() ![]() | |
发表期刊 | ASTROPHYSICS AND SPACE SCIENCE (IF:1.885[JCR-2017],1.554[5-Year]) |
2011-03 | |
卷号 | 332期号:1页码:81-89 |
DOI | 10.1007/s10509-010-0505-9 |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Sun: Loop Eruption Sun: Flux Emergence Sun: Coronal Mass Ejections (Cmes) |
摘要 | By using the multi-wavelength observations from the Solar Terrestrial Relations Observatory (STEREO), the Solar and Heliospheric Observatory (SOHO), the Transition Region and Coronal Explorer (TRACE) and the HINODE, we study a coronal mass ejection (CME) and associated coronal dimming occurred on 2009 December 13, as a consequence of the expansion and eruption of EUV loops. The activities were probably triggered by the new flux emergence and the convergence motions, which were evident in the magnetograms from Michelson Doppler Imager (MDI) on the SOHO. The emergence led to the destabilization and eruption of the preexistent flux rope, which was highly-sheared over the polarity inversion line. Driven by the ejection of the flux rope, the overlying loops initially slowly rose and then erupted. As a result, two coronal dimming regions formed at the footprints of the loops and a B1.9 flare, about half an hour later, occurred in the eruptive region near one foot of the eruptive loops. The CME had a very close temporal and spatial relationship to the expanding loops, and it is very likely that the CME directly developed from the eruptive loops. The CME mass calculated from the EUV dimming was of the same order of the typical CME mass, suggesting that the dimming region supplied major of the mass for the CME. The kinematic evolution of the CME was basically consistent with the three-phases scenario: the initiation phase, impulsive acceleration phase, and propagation phase. The onset of the CME could be well explained by the emerging flux trigger mechanism. |
项目资助者 | 973 Program [2011CB811400] ; Natural Science Foundation of China [10973038, 40636031] ; Scientific Application Foundation of Yunnan Province [2007A112M, 2007A115M] |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 0004-640X |
URL | 查看原文 |
归档日期 | 2011-02-21 |
WOS记录号 | WOS:000287981300009 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | RAY TELESCOPE XRT ; SOLAR-FLARE MYTH ; MAGNETIC-FLUX ; EMERGING FLUX ; INTERCONNECTING LOOPS ; MISSION ; CMES ; DISAPPEARANCES ; INITIATION ; FILAMENT |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/6183 |
专题 | 太阳物理研究组 |
通讯作者 | Zheng, RS (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China. |
作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, China 2.Graduate School of Chinese Academy of Sciences, Beijing, 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 | Zheng RS,Jiang YC,Yang LH,et al. The coronal mass ejection associated with the loop eruption and coronal dimmings on 2009 December 13[J]. ASTROPHYSICS AND SPACE SCIENCE,2011,332(1):81-89. |
APA | Zheng RS,Jiang YC,Yang LH,Bi Y,&Zheng, RS .(2011).The coronal mass ejection associated with the loop eruption and coronal dimmings on 2009 December 13.ASTROPHYSICS AND SPACE SCIENCE,332(1),81-89. |
MLA | Zheng RS,et al."The coronal mass ejection associated with the loop eruption and coronal dimmings on 2009 December 13".ASTROPHYSICS AND SPACE SCIENCE 332.1(2011):81-89. |
条目包含的文件 | ||||||
文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
The coronal mass eje(567KB) | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论