Magnetic helicity accumulation and tilt angle evolution of newly emerging active regions
文献类型:期刊论文
作者 | Yang, S.1,2; Zhang, H.1; Buechner, J.2 |
刊名 | ASTRONOMY & ASTROPHYSICS
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出版日期 | 2009-07-01 |
卷号 | 502期号:1页码:333-340 |
关键词 | Sun: magnetic fields Sun: activity |
英文摘要 | Context. It has been known for years that there is a general dominance of negative (positive) helicity of active regions (ARs) in the northern (southern) solar hemisphere. For a better understanding of the role of helicity in the evolution of active regions, it is necessary to know more about the accumulation of helicity during the emergence of active regions. In particular, different conclusions were drawn in the past about the relationship between the accumulated helicity and the writhe of active regions. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000268535800029 |
源URL | [http://ir.bao.ac.cn/handle/114a11/7595] ![]() |
专题 | 国家天文台_太阳物理研究部 |
作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 2.Max Planck Inst Solar Syst Res, D-37191 Katlenburg Lindau, Germany |
推荐引用方式 GB/T 7714 | Yang, S.,Zhang, H.,Buechner, J.. Magnetic helicity accumulation and tilt angle evolution of newly emerging active regions[J]. ASTRONOMY & ASTROPHYSICS,2009,502(1):333-340. |
APA | Yang, S.,Zhang, H.,&Buechner, J..(2009).Magnetic helicity accumulation and tilt angle evolution of newly emerging active regions.ASTRONOMY & ASTROPHYSICS,502(1),333-340. |
MLA | Yang, S.,et al."Magnetic helicity accumulation and tilt angle evolution of newly emerging active regions".ASTRONOMY & ASTROPHYSICS 502.1(2009):333-340. |
入库方式: OAI收割
来源:国家天文台
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