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A SOLAR TYPE II RADIO BURST FROM CORONAL MASS EJECTION-CORONAL RAY INTERACTION: SIMULTANEOUS RADIO AND EXTREME ULTRAVIOLET IMAGING
Chen, Yao1,2; Du, Guohui1,2; Feng, Li3; Feng, Shiwei1,2; Kong, Xiangliang1,2; Guo, Fan4; Wang, Bing1,2; Li, Gang5,6
2014-05-20
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume787Issue:1Pages:0
AbstractSimultaneous radio and extreme ultraviolet (EUV)/white-light imaging data are examined for a solar type II radio burst occurring on 2010 March 18 to deduce its source location. Using a bow-shock model, we reconstruct the three-dimensional EUV wave front (presumably the type-II-emitting shock) based on the imaging data of the two Solar TErrestrial RElations Observatory spacecraft. It is then combined with the Nancay radio imaging data to infer the three-dimensional position of the type II source. It is found that the type II source coincides with the interface between the coronal mass ejection (CME) EUV wave front and a nearby coronal ray structure, providing evidence that the type II emission is physically related to the CME-ray interaction. This result, consistent with those of previous studies, is based on simultaneous radio and EUV imaging data for the first time.
KeywordShock Waves Sun: Corona Sun: Coronal Mass Ejections (Cmes) Sun: Radio Radiation
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1088/0004-637X/787/1/59
WOS KeywordNOVEMBER 2003 ; SOHO MISSION ; SHOCK ; ELECTRONS ; ACCELERATION ; WAVES ; DIAGNOSTICS ; DYNAMICS ; FLARE ; CMES
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Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000335924200059
Citation statistics
Cited Times:30[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/10626
Collection太阳高能及相关物理过程研究团组
Affiliation1.Shandong Univ, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Weihai 264209, Peoples R China
2.Shandong Univ, Inst Space Sci, Weihai 264209, Peoples R China
3.Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210008, Jiangsu, Peoples R China
4.Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA
5.Univ Alabama, Dept Space Sci, Huntsville, AL 35899 USA
6.Univ Alabama, CSPAR, Huntsville, AL 35899 USA
Recommended Citation
GB/T 7714
Chen, Yao,Du, Guohui,Feng, Li,et al. A SOLAR TYPE II RADIO BURST FROM CORONAL MASS EJECTION-CORONAL RAY INTERACTION: SIMULTANEOUS RADIO AND EXTREME ULTRAVIOLET IMAGING[J]. ASTROPHYSICAL JOURNAL,2014,787(1):0.
APA Chen, Yao.,Du, Guohui.,Feng, Li.,Feng, Shiwei.,Kong, Xiangliang.,...&Li, Gang.(2014).A SOLAR TYPE II RADIO BURST FROM CORONAL MASS EJECTION-CORONAL RAY INTERACTION: SIMULTANEOUS RADIO AND EXTREME ULTRAVIOLET IMAGING.ASTROPHYSICAL JOURNAL,787(1),0.
MLA Chen, Yao,et al."A SOLAR TYPE II RADIO BURST FROM CORONAL MASS EJECTION-CORONAL RAY INTERACTION: SIMULTANEOUS RADIO AND EXTREME ULTRAVIOLET IMAGING".ASTROPHYSICAL JOURNAL 787.1(2014):0.
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