中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
NLTE modelling of the flaring atmosphere above sunspot

文献类型:期刊论文

作者Berlicki, A.1,2; Heinzel, P.3; Schmieder, B.1; Li, H.4
刊名ASTRONOMY & ASTROPHYSICS
出版日期2008-10-01
卷号490期号:1页码:315-324
关键词Sun: atmosphere Sun: flares sunspots line: profiles
ISSN号0004-6361
英文摘要Aims. We performed an analysis of the solar flaring atmosphere above sunspots. During the flare on October 20, 2003 many flaring structures were observed projected onto the sunspots. We analysed the H alpha and Ca II line profiles emitted by the ribbons partially overlapping the sunspots. In the penumbra, the line intensity in the far wings is lower than in a typical quiet Sun profile but the core emission of H alpha and Ca II lines is typical for flares. We tried to find the structure of the flare observed above the sunspot penumbra using the observations of these chromospheric line profiles.
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]HYDROGEN LYMAN LINES ; WHITE-LIGHT FLARE ; 1982 JUNE 15 ; GRADUAL PHASE ; SOLAR-FLARES ; FILAMENT OBSERVATIONS ; QUIET-SUN ; H-ALPHA ; LOOPS ; DIAGNOSTICS
收录类别SCI
语种英语
WOS记录号WOS:000259966600033
公开日期2011-12-29
源URL[http://159.226.72.40/handle/332002/1893]  
专题紫金山天文台_太阳高能及相关物理过程研究团组
作者单位1.LESIA, Sect Meudon, Observ Paris, F-92195 Meudon, France
2.Univ Wroclaw, Astron Inst, PL-51622 Wroclaw, Poland
3.Acad Sci Czech Republic, Inst Astron, CS-25165 Ondrejov, Czech Republic
4.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
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Berlicki, A.,Heinzel, P.,Schmieder, B.,et al. NLTE modelling of the flaring atmosphere above sunspot[J]. ASTRONOMY & ASTROPHYSICS,2008,490(1):315-324.
APA Berlicki, A.,Heinzel, P.,Schmieder, B.,&Li, H..(2008).NLTE modelling of the flaring atmosphere above sunspot.ASTRONOMY & ASTROPHYSICS,490(1),315-324.
MLA Berlicki, A.,et al."NLTE modelling of the flaring atmosphere above sunspot".ASTRONOMY & ASTROPHYSICS 490.1(2008):315-324.

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来源:紫金山天文台

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