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Anomalous resistivity in beam-return currents and hard-X ray spectra of solar flares
Xu, L.1,2; Chen, L.1; Wu, D. J.1
2013-02-01
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume550Pages:A63-A63
Corresponding Author吴德金
AbstractContext. Observations of hard-X ray (HXR) spectra from solar flares show that there is noncollisional energy loss when energetic beam electrons are transported along the flare loop from their acceleration site above the looptop in the corona to the loop footpoints in the chromosphere.
KeywordSun: Flares Sun: X-Rays, Gamma Rays Plasmas Acceleration Of Particles
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1051/0004-6361/201220253
WOS KeywordCURRENT SYSTEMS ; FOOTPOINT SOURCES ; EMISSION ; ENERGY ; ELECTRONS ; GENERATION ; BURSTS ; RHESSI
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000314879700063
Citation statistics
Cited Times:4[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/9868
Collection太阳和太阳系等离子体研究团组
Affiliation1.Chinese Acad Sci, Purple Mt Observ, Nanjing, Jiangsu, Peoples R China
2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
Recommended Citation
GB/T 7714
Xu, L.,Chen, L.,Wu, D. J.. Anomalous resistivity in beam-return currents and hard-X ray spectra of solar flares[J]. ASTRONOMY & ASTROPHYSICS,2013,550:A63-A63.
APA Xu, L.,Chen, L.,&Wu, D. J..(2013).Anomalous resistivity in beam-return currents and hard-X ray spectra of solar flares.ASTRONOMY & ASTROPHYSICS,550,A63-A63.
MLA Xu, L.,et al."Anomalous resistivity in beam-return currents and hard-X ray spectra of solar flares".ASTRONOMY & ASTROPHYSICS 550(2013):A63-A63.
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