中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
THE CAUSE OF THE WEAK SOLAR CYCLE 24

文献类型:期刊论文

作者Jiang, J.1; Cameron, R. H.2; Schuessler, M.2
刊名ASTROPHYSICAL JOURNAL LETTERS
出版日期2015-07-20
卷号808期号:1
关键词Sun: activity Sun: magnetic fields
英文摘要The ongoing 11 year cycle of solar activity is considerably less vigorous than the three cycles before. It was preceded by a very deep activity minimum with a low polar magnetic flux, the source of the toroidal field responsible for solar magnetic activity in the subsequent cycle. Simulation of the evolution of the solar surface field shows that the weak polar fields and thus the weakness of the present cycle 24 are mainly caused by a number of bigger bipolar regions emerging at low latitudes with a "wrong" (i.e., opposite to the majority for this cycle) orientation of their magnetic polarities in the north-south direction, which impaired the growth of the polar field. These regions had a particularly strong effect since they emerged within +/- 10 degrees latitude from the solar equator.
收录类别SCI
语种英语
WOS记录号WOS:000358778900028
源URL[http://ir.bao.ac.cn/handle/114a11/5650]  
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, Key Lab Solar Act, Beijing 100012, Peoples R China
2.Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany
推荐引用方式
GB/T 7714
Jiang, J.,Cameron, R. H.,Schuessler, M.. THE CAUSE OF THE WEAK SOLAR CYCLE 24[J]. ASTROPHYSICAL JOURNAL LETTERS,2015,808(1).
APA Jiang, J.,Cameron, R. H.,&Schuessler, M..(2015).THE CAUSE OF THE WEAK SOLAR CYCLE 24.ASTROPHYSICAL JOURNAL LETTERS,808(1).
MLA Jiang, J.,et al."THE CAUSE OF THE WEAK SOLAR CYCLE 24".ASTROPHYSICAL JOURNAL LETTERS 808.1(2015).

入库方式: OAI收割

来源:国家天文台

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