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Two Quasi-periodic Fast-propagating Magnetosonic Wave Events Observed in Active Region NOAA 11167
Miao YH(苗玉虎)1,2; Liu Y(刘煜)2; Elmhamdi,A.3; Kordi,A. S.3; Shen YD(申远灯)2; Al-Shammari, Rehab3; Al-Mosabeh, Khaled3; Jiang, Chaowei1; Yuan, Ding1
通讯作者Miao, Yuhu([email protected])
发表期刊ASTROPHYSICAL JOURNAL
2020-02-01
卷号889期号:2页码:14
DOI10.3847/1538-4357/ab655f
产权排序第2完成单位
收录类别SCI
关键词Solar corona Magnetohydrodynamics Solar flares Solar extreme ultraviolet emission Solar active regions Solar coronal waves Space plasmas
摘要We report a detailed observational study of two quasi-periodic fast-propagating (QFP) magnetosonic wave events that occurred on 2011 March 9 and 10, respectively. Interestingly, both the events have two wave trains (WTs): a strong main one (WT-1) and a small and weak secondary one (WT-2). Peculiar and common characteristics of the two events are observed, namely, (1) the two QFP waves are accompanied with brightenings during the whole stage of the eruptions; (2) both the two main WTs are nearly propagating along the same direction; (3) extreme-ultraviolet (EUV) waves are found to be associated with the two events. Investigating various aspects of the target events, we argue that (1) the second event is accompanied with a flux rope eruption during the whole stage; (2) the second event eruption produces a new filament-like dark feature; (3) the ripples of the two WT-2 QFP waves seem to result from different triggering mechanisms. Based on the obtained observational results, we propose that the funnel-like coronal loop system is indeed playing an important role in the two WT-1 QFP waves. The development of the second WT-2 QFP wave can be explained as due to the dispersion of the main EUV front. The coexistence of the two events offers thereby a significant opportunity to reveal what driving mechanisms and structures are tightly related to the waves.
资助项目National Natural Science Foundation of China (NSFC)[11803005] ; National Natural Science Foundation of China (NSFC)[41731067] ; Shenzhen Technology Project[JCYJ20180306172239618] ; Fundamental Research Funds for the Central Universities[HIT.BRETIV.201901] ; National Scientific Foundation of China[11533009, 11973086] ; Deanship of Scientific Research at King Saud University through research group[RG-1440-092] ; One Belt and One Road project of the West Light Foundation, CAS
项目资助者National Natural Science Foundation of China (NSFC)[11803005, 41731067] ; Shenzhen Technology Project[JCYJ20180306172239618] ; Fundamental Research Funds for the Central Universities[HIT.BRETIV.201901] ; National Scientific Foundation of China[11533009, 11973086] ; Deanship of Scientific Research at King Saud University through research group[RG-1440-092] ; One Belt and One Road project of the West Light Foundation, CAS
语种英语
学科领域天文学 ; 太阳与太阳系 ; 太阳物理学
文章类型Article
出版者IOP PUBLISHING LTD
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS记录号WOS:000525683300001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]ULTRAVIOLET IMAGING TELESCOPE ; SOHO/EIT OBSERVATIONS ; MORETON WAVES ; EUV WAVES ; MHD WAVES ; EIT WAVES ; SOLAR ; OSCILLATIONS ; SIMULATION
引用统计
被引频次:10[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/22299
专题选址与日冕观测组
作者单位1.Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen 518055, People's Republic of China
2.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China
3.Department of Physics and Astronomy, King Saud University, P.O. Box 2455, Riyadh 11451, Saudi Arabia
第一作者单位中国科学院云南天文台
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Miao YH,Liu Y,Elmhamdi,A.,et al. Two Quasi-periodic Fast-propagating Magnetosonic Wave Events Observed in Active Region NOAA 11167[J]. ASTROPHYSICAL JOURNAL,2020,889(2):14.
APA Miao YH.,Liu Y.,Elmhamdi,A..,Kordi,A. S..,Shen YD.,...&Yuan, Ding.(2020).Two Quasi-periodic Fast-propagating Magnetosonic Wave Events Observed in Active Region NOAA 11167.ASTROPHYSICAL JOURNAL,889(2),14.
MLA Miao YH,et al."Two Quasi-periodic Fast-propagating Magnetosonic Wave Events Observed in Active Region NOAA 11167".ASTROPHYSICAL JOURNAL 889.2(2020):14.
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