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![]() ![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
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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 |
推荐引用方式 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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