Solar surface rotation: N-S asymmetry and recent speed-up
文献类型:期刊论文
作者 | Zhang, L.1,2![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
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出版日期 | 2015-03-01 |
卷号 | 575 |
关键词 | Sun: activity Sun: flares Sun: rotation sunspots Sun: evolution |
英文摘要 | Context. The relation between solar surface rotation and sunspot activity is still not fully resolved. The sunspot activity has been significantly reduced in solar cycle 24, and several solar activity indices and flux measurements experienced unprecedentedly low levels during the last solar minimum. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000350249100101 |
源URL | [http://ir.bao.ac.cn/handle/114a11/5743] ![]() |
专题 | 国家天文台_光学天文研究部 |
作者单位 | 1.Univ Oulu, Dept Phys, ReSoLVE Ctr Excellence, Oulu 90014, Finland 2.Chinese Acad Sci, Key Lab Solar Act, Natl Astron Observ, Beijing 100875, Peoples R China 3.Univ Oulu, Sodankyla Geophys Observ, Oulu 90014, Finland |
推荐引用方式 GB/T 7714 | Zhang, L.,Mursula, K.,Usoskin, I.. Solar surface rotation: N-S asymmetry and recent speed-up[J]. ASTRONOMY & ASTROPHYSICS,2015,575. |
APA | Zhang, L.,Mursula, K.,&Usoskin, I..(2015).Solar surface rotation: N-S asymmetry and recent speed-up.ASTRONOMY & ASTROPHYSICS,575. |
MLA | Zhang, L.,et al."Solar surface rotation: N-S asymmetry and recent speed-up".ASTRONOMY & ASTROPHYSICS 575(2015). |
入库方式: OAI收割
来源:国家天文台
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