中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The evolution of arch filament systems and moving magnetic features around a sunspot

文献类型:期刊论文

作者Ma, Li1,2; Zhou, Wangping1,2; Zhou, Guiping2; Zhang, Jun2
刊名ASTRONOMY & ASTROPHYSICS
出版日期2015-11-01
卷号583
关键词sunspots Sun: filaments, prominences Sun: magnetic fields
英文摘要Context. Arch filament systems (AFSs) are usually considered as the chromospheric manifestations of the emerging flux regions (EFRs) seen in Ha observations. Moving magnetic features (MIMEO look similar to EFRs in magnetograms, but often appear in the decaying phase of an active region (AR) and behave differently from EFRs. A possible relation between AFS and MMF would be important for revealing a common mechanism for building up basic structures on the Sun.
收录类别SCI
语种英语
WOS记录号WOS:000365072200006
源URL[http://ir.bao.ac.cn/handle/114a11/5527]  
专题国家天文台_太阳物理研究部
作者单位1.Nanjing Univ Informat Sci & Technol, Sch Informat Sci & Control, CICAEET, Nanjing 210044, Jiangsu, Peoples R China
2.Chinese Acad Sci, Key Lab Solar Act, Natl Astron Observ, Beijing 100012, Peoples R China
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GB/T 7714
Ma, Li,Zhou, Wangping,Zhou, Guiping,et al. The evolution of arch filament systems and moving magnetic features around a sunspot[J]. ASTRONOMY & ASTROPHYSICS,2015,583.
APA Ma, Li,Zhou, Wangping,Zhou, Guiping,&Zhang, Jun.(2015).The evolution of arch filament systems and moving magnetic features around a sunspot.ASTRONOMY & ASTROPHYSICS,583.
MLA Ma, Li,et al."The evolution of arch filament systems and moving magnetic features around a sunspot".ASTRONOMY & ASTROPHYSICS 583(2015).

入库方式: OAI收割

来源:国家天文台

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