中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The radio signature of magnetic reconnection for the M-class flare of 2004 November 1

文献类型:期刊论文

作者Huang, Guangli1; Ji, Haisheng1; Wu, Guiping1,2
刊名ASTROPHYSICAL JOURNAL LETTERS
出版日期2008-01-10
卷号672期号:2页码:L131-L134
关键词Sun : flares Sun : magnetic fields Sun : particle emission
英文摘要In this Letter, we present radio diagnostics for the magnetic field and the density distribution of nonthermal electrons in the microwave source of the M1.1 flare of 2004 November 1. We calculate the nonthermal gyrosynchrotron radiation using observations made at the Nobeyama Radio Observatory to get the longitudinal magnetic field and the magnitude of the transverse magnetic field. The computed longitudinal magnetic field at two hard X-ray footpoints has opposite polarities, which basically agrees with SOHO MDI observations. The main finding is that the magnitude of the transverse magnetic field summed around the magnetic neutral line of the SOHO MDI magnetogram has a short-term impulsive increase during the rising phase of the flare. We propose that the increase of the transverse magnetic field may be considered evidence of the magnetic reconnection process in this flare. The computed mean angle between the magnetic field and line of sight decreases steadily during the flare, clearly indicating the reconfiguration of the magnetic field, presumably the relaxation of the sheared magnetic field. Moreover, the calculated density of nonthermal electrons increases from footpoints to looptop, while the spectral index calculated by the Nobeyama Radio Heliograph at 17 and 34 GHz decreases from footpoints ( soft) to looptop ( hard), which may confirm that the reconnection site is close to the looptop source.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]SOLAR MICROWAVE-BURSTS ; FIELD ; NOBEYAMA ; RELAXATION ; ELECTRONS ; LINE
收录类别SCI
语种英语
WOS记录号WOS:000255232300012
公开日期2011-12-30
源URL[http://159.226.72.40/handle/332002/2037]  
专题紫金山天文台_太阳活动的多波段观测研究团组
作者单位1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
2.SE Univ, Dept Phys, Nanjing 210096, Peoples R China
推荐引用方式
GB/T 7714
Huang, Guangli,Ji, Haisheng,Wu, Guiping. The radio signature of magnetic reconnection for the M-class flare of 2004 November 1[J]. ASTROPHYSICAL JOURNAL LETTERS,2008,672(2):L131-L134.
APA Huang, Guangli,Ji, Haisheng,&Wu, Guiping.(2008).The radio signature of magnetic reconnection for the M-class flare of 2004 November 1.ASTROPHYSICAL JOURNAL LETTERS,672(2),L131-L134.
MLA Huang, Guangli,et al."The radio signature of magnetic reconnection for the M-class flare of 2004 November 1".ASTROPHYSICAL JOURNAL LETTERS 672.2(2008):L131-L134.

入库方式: OAI收割

来源:紫金山天文台

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