AN EXTREME ULTRAVIOLET WAVE ASSOCIATED WITH A MICRO-SIGMOID ERUPTION | |
Zheng RS(郑瑞生); Jiang YC(姜云春); Yang JY(杨家艳); Bi Y(毕以); Hong JC(洪俊超); Yang D(杨丹); Yang B(杨波) | |
刊名 | ASTROPHYSICAL JOURNAL LETTERS |
2012-07-10 | |
卷号 | 753期号:2页码:29-35 |
关键词 | Sun: activity Sun: corona Sun: filaments prominences |
ISSN号 | 2041-8205 |
通讯作者 | Zheng, RS (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Astron Observ, Kunming 650011, Peoples R China. |
产权排序 | 第一完成单位 |
英文摘要 | Taking advantage of the high temporal and spatial resolution of the Solar Dynamics Observatory (SDO) observations, we present an extreme ultraviolet (EUV) wave associated with a micro-sigmoid eruption on 2010 October 21. The micro-sigmoid underwent a typical "sigmoid-to-arcade" evolution via tether-cutting reconnection, accompanied by a B1.7 flare, a filament eruption, and coronal twin dimmings. In the eruption, the newly formed sigmoidal loops expanded quickly, and the expansion likely triggered an EUV wave. The wave onset was nearly simultaneous with the start of the eruption and the associated flare. The wave had a nearly circular front and propagated at a constant velocity of 270-350 km s(-1) with very little angular dependence. Remarkably, in some direction, the wave encountered a small loop and refracted at a higher speed. All the results provide evidences that the wave was a fast-mode magnetohydrodynamic (MHD) wave. Owing to the close temporal and spatial relationship between the wave and the expanding loops, we believe that the wave was most likely triggered by the fast expansion of the newly formed sigmoidal loops, which evolved into the leading front of the invisible micro-coronal mass ejection. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | CORONAL MASS EJECTION ; EIT WAVES ; ACTIVE-REGION ; SOLAR CORONA ; PROPAGATING DISTURBANCE ; SOHO/EIT OBSERVATIONS ; NUMERICAL-SIMULATION ; MORETON WAVES ; YOHKOH SXT ; MHD WAVES |
收录类别 | SCI |
原文出处 | http://iopscience.iop.org/article/10.1088/2041-8205/753/2/L29/meta |
语种 | 英语 |
WOS记录号 | WOS:000305902700004 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/6197] |
专题 | 云南天文台_太阳物理研究组 |
作者单位 | National Astronomical Observatories/Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China |
推荐引用方式 GB/T 7714 | Zheng RS,Jiang YC,Yang JY,et al. AN EXTREME ULTRAVIOLET WAVE ASSOCIATED WITH A MICRO-SIGMOID ERUPTION[J]. ASTROPHYSICAL JOURNAL LETTERS,2012,753(2):29-35. |
APA | Zheng RS.,Jiang YC.,Yang JY.,Bi Y.,Hong JC.,...&Yang B.(2012).AN EXTREME ULTRAVIOLET WAVE ASSOCIATED WITH A MICRO-SIGMOID ERUPTION.ASTROPHYSICAL JOURNAL LETTERS,753(2),29-35. |
MLA | Zheng RS,et al."AN EXTREME ULTRAVIOLET WAVE ASSOCIATED WITH A MICRO-SIGMOID ERUPTION".ASTROPHYSICAL JOURNAL LETTERS 753.2(2012):29-35. |
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