中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Observations of a Fast-mode Magnetosonic Wave Propagating along a Curving Coronal Loop on 2011 November 11

文献类型:期刊论文

作者Qu, Z. N.1,2; Jiang, L. Q.1; Chen, S. L.1
刊名ASTROPHYSICAL JOURNAL
出版日期2017-12-10
卷号851期号:1页码:9
ISSN号0004-637X
关键词Sun: activity Sun: coronal mass ejections (CMEs) Sun: filaments, prominences Sun: flares
DOI10.3847/1538-4357/aa9beb
英文摘要The detailed analysis of an interesting quasi-periodic fast-propagating (QFP) magnetosonic wave is presented using high-resolution observations taken by the Solar Dynamic Observatory. The QFP wave occurred over the west solar limb during the fast eruption phase of a nearby prominence. It propagated along a group of curving coronal loop and manifested two types of wave trains that showed different morphologies and propagation characteristics. The wavefronts of the first type wave trains are relatively broad, and they changed their propagation direction when they pass through the turning part of the guiding loop. On the contrary, the wavefronts of the other type wave trains are narrow, and their propagation did not affected by geometric changes of the guiding loop. Measurements indicate that the average speeds of the broad (narrow) wave trains is 305(343) km s(-1), and the period of the wave trains ranges from 54 to 458 s. We propose that the narrow wave trains may manifest the leakage of the wave trains from the guiding coronal loop, or were guided by another group of invisible coronal loop. In addition, the projection effect and weak magnetic field strength of the guiding coronal loop are proposed to explain the slow wave speed.
WOS关键词TIME-SERIES ANALYSIS ; MORETON WAVES ; SOLAR CORONA ; ALFVEN WAVES ; EIT WAVES ; OSCILLATIONS ; DECOMPOSITION ; JETS ; SDO
资助项目National Natural Science Foundation of China[11503082] ; National Natural Science Foundation of China[11403097] ; National Natural Science Foundation of China[11633008] ; National Natural Science Foundation of China[11773068] ; National Natural Science Foundation of China (NSFC)[U1631108] ; Chinese Academy of Sciences (CAS)[U1631108] ; open research program of Key Laboratory of Solar Activity of Chinese Academy of Sciences[KLSA201711] ; research fund of Sichuan University of Science and Engineering[2015RC42] ; research fund of Sichuan University of Science and Engineering[2015RC43] ; Yunnan Science Foundation[2015FB191] ; Yunnan Science Foundation[2017FB006] ; Youth Innovation Promotion Association of Chinese Academy of Sciences[2014047]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000417808300001
资助机构National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; open research program of Key Laboratory of Solar Activity of Chinese Academy of Sciences ; open research program of Key Laboratory of Solar Activity of Chinese Academy of Sciences ; research fund of Sichuan University of Science and Engineering ; research fund of Sichuan University of Science and Engineering ; Yunnan Science Foundation ; Yunnan Science Foundation ; Youth Innovation Promotion Association of Chinese Academy of Sciences ; Youth Innovation Promotion Association of Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; open research program of Key Laboratory of Solar Activity of Chinese Academy of Sciences ; open research program of Key Laboratory of Solar Activity of Chinese Academy of Sciences ; research fund of Sichuan University of Science and Engineering ; research fund of Sichuan University of Science and Engineering ; Yunnan Science Foundation ; Yunnan Science Foundation ; Youth Innovation Promotion Association of Chinese Academy of Sciences ; Youth Innovation Promotion Association of Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; open research program of Key Laboratory of Solar Activity of Chinese Academy of Sciences ; open research program of Key Laboratory of Solar Activity of Chinese Academy of Sciences ; research fund of Sichuan University of Science and Engineering ; research fund of Sichuan University of Science and Engineering ; Yunnan Science Foundation ; Yunnan Science Foundation ; Youth Innovation Promotion Association of Chinese Academy of Sciences ; Youth Innovation Promotion Association of Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; open research program of Key Laboratory of Solar Activity of Chinese Academy of Sciences ; open research program of Key Laboratory of Solar Activity of Chinese Academy of Sciences ; research fund of Sichuan University of Science and Engineering ; research fund of Sichuan University of Science and Engineering ; Yunnan Science Foundation ; Yunnan Science Foundation ; Youth Innovation Promotion Association of Chinese Academy of Sciences ; Youth Innovation Promotion Association of Chinese Academy of Sciences
源URL[http://ir.bao.ac.cn/handle/114a11/37350]  
专题中国科学院国家天文台
通讯作者Qu, Z. N.
作者单位1.Sichuan Univ Sci & Engn, Sch Phys & Elect Engn, Zigong 643000, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China
推荐引用方式
GB/T 7714
Qu, Z. N.,Jiang, L. Q.,Chen, S. L.. Observations of a Fast-mode Magnetosonic Wave Propagating along a Curving Coronal Loop on 2011 November 11[J]. ASTROPHYSICAL JOURNAL,2017,851(1):9.
APA Qu, Z. N.,Jiang, L. Q.,&Chen, S. L..(2017).Observations of a Fast-mode Magnetosonic Wave Propagating along a Curving Coronal Loop on 2011 November 11.ASTROPHYSICAL JOURNAL,851(1),9.
MLA Qu, Z. N.,et al."Observations of a Fast-mode Magnetosonic Wave Propagating along a Curving Coronal Loop on 2011 November 11".ASTROPHYSICAL JOURNAL 851.1(2017):9.

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来源:国家天文台

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