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Observations of a Fast-mode Magnetosonic Wave Propagating along a Curving Coronal Loop on 2011 November 11
Qu, Z. N.1,2; Jiang, L. Q.1; Chen, S. L.1
2017-12-10
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume851Issue:1Pages:9
AbstractThe 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.
KeywordSun: activity Sun: coronal mass ejections (CMEs) Sun: filaments, prominences Sun: flares
Funding OrganizationNational 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
DOI10.3847/1538-4357/aa9beb
WOS KeywordTIME-SERIES ANALYSIS ; MORETON WAVES ; SOLAR CORONA ; ALFVEN WAVES ; EIT WAVES ; OSCILLATIONS ; DECOMPOSITION ; JETS ; SDO
Language英语
Funding ProjectNational 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]
Funding OrganizationNational 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
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000417808300001
PublisherIOP PUBLISHING LTD
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/37351
Collection中国科学院国家天文台
Corresponding AuthorQu, Z. N.
Affiliation1.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
Recommended Citation
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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