YNAO OpenIR  > 选址与日冕观测组
CME-Driven and Flare-Ignited Fast Magnetosonic Waves Detected in a Solar Eruption
Zhou XP(周新平)1,2,3,4; Shen YD(申远灯)1,2,3,4; Su, Jiangtao3,4; Tang ZH(汤泽浩)1,4; Zhou CR(周承瑞)1,4; Duan YD(段雅丹)1,4; Tan S(谭宋)1,4
发表期刊SOLAR PHYSICS
2021-11
卷号296期号:11
DOI10.1007/s11207-021-01913-2
产权排序第1完成单位
收录类别SCI
关键词Waves magnetohydrodynamic Magnetic fields corona Coronal seismology
摘要

We present Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) observation of three types of fast-mode, propagating, magnetosonic waves in a GOES C3.0 flare on 23 April 2013, which was accompanied by a prominence eruption and a broad coronal mass ejection (CME). During the fast-rising phase of the prominence, a large-scale, dome-shaped, extreme-ultraviolet (EUV) wave firstly formed ahead of the CME bubble and propagated at a speed of about 430 km s(-1) in the CME's lateral direction. One can identify the separation process of the EUV wave from the CME bubble. The reflection effect of the on-disk counterpart of this EUV wave was also observed when it interacted with a remote active region. Six minutes after the first appearance of the EUV wave, a large-scale, quasi-periodic EUV train with a period of about 120 seconds, which emanated from the flare epicenter and propagated outward at an average speed up to 1100 km s(-1), appeared inside the CME bubble. In addition, another narrow, quasi-periodic EUV wave train, which also emanated from the flare epicenter, propagated at a speed of about 475 km s(-1) and with a period of about 110 seconds, was observed along a closed-loop system connecting two adjacent active regions. We propose that all of the observed waves are fast-mode magnetosonic waves, in which the large-scale, dome-shaped EUV wave ahead of the CME bubble was driven by the expansion of the CME bubble, while the large-scale, quasi-periodic EUV train within the CME bubble and the narrow quasi-periodic EUV wave train along the closed-loop system were excited by the intermittent energy-releasing process in the flare. Coronal seismology application and energy carried by the waves are also estimated based on the measured wave parameters.

资助项目National Key R&D Program of China[2019YFA0405000] ; Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[12173083] ; Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11922307] ; Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11773068] ; Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11633008] ; Yunnan Science Foundation for Distinguished Young Scholars[202101AV070004] ; Specialized Research Fund for State Key Laboratories ; Open Research Program of CAS Key Laboratory of Solar Activity[KLSA202017] ; West Light Foundation of Chinese Academy of SciencesChinese Academy of Sciences ; Yunnan Science Foundation[2017FB006]
项目资助者National Key R&D Program of China[2019YFA0405000] ; Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[12173083, 11922307, 11773068, 11633008] ; Yunnan Science Foundation for Distinguished Young Scholars[202101AV070004] ; Specialized Research Fund for State Key Laboratories ; Open Research Program of CAS Key Laboratory of Solar Activity[KLSA202017] ; West Light Foundation of Chinese Academy of SciencesChinese Academy of Sciences ; Yunnan Science Foundation[2017FB006]
语种英语
学科领域天文学 ; 太阳与太阳系 ; 太阳物理学
学科门类理学 ; 理学::天文学
文章类型Article
出版者SPRINGER
出版地VAN GODEWIJCKSTRAAT 30, 3311 GZ DORDRECHT, NETHERLANDS
ISSN0038-0938
URL查看原文
WOS记录号WOS:000720040700001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]CORONAL MASS EJECTION ; LARGE-SCALE WAVES ; EIT WAVES ; MORETON WAVES ; RADIO ; SHOCK ; MULTIWAVELENGTH ; OSCILLATIONS
引用统计
被引频次:14[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/24678
专题选址与日冕观测组
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650011, China;
2.State Key Laboratory of Space Weather, Chinese Academy of Sciences, Beijing, 100190, China;
3.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China;
4.University of Chinese Academy of Sciences, Beijing, 10049, 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
Zhou XP,Shen YD,Su, Jiangtao,et al. CME-Driven and Flare-Ignited Fast Magnetosonic Waves Detected in a Solar Eruption[J]. SOLAR PHYSICS,2021,296(11).
APA 周新平.,申远灯.,Su, Jiangtao.,汤泽浩.,周承瑞.,...&谭宋.(2021).CME-Driven and Flare-Ignited Fast Magnetosonic Waves Detected in a Solar Eruption.SOLAR PHYSICS,296(11).
MLA 周新平,et al."CME-Driven and Flare-Ignited Fast Magnetosonic Waves Detected in a Solar Eruption".SOLAR PHYSICS 296.11(2021).
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
CME-Driven and Flare(5139KB)期刊论文出版稿开放获取CC BY-NC-SA浏览 请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[周新平]的文章
[申远灯]的文章
[Su, Jiangtao]的文章
百度学术
百度学术中相似的文章
[周新平]的文章
[申远灯]的文章
[Su, Jiangtao]的文章
必应学术
必应学术中相似的文章
[周新平]的文章
[申远灯]的文章
[Su, Jiangtao]的文章
相关权益政策
暂无数据
收藏/分享
文件名: CME-Driven and Flare-Ignited Fast Magnetosonic Waves Detected in a Solar Eruption.pdf
格式: Adobe PDF
所有评论 (0)
暂无评论
 

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。