中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The tangential discontinuous surface of velocity in solar chromosphere

文献类型:期刊论文

作者Hu WR(胡文瑞); Zhang HQ; Chen JM
刊名Science in China Series A-Mathematics Physics Astronomy
出版日期1991
卷号34期号:11页码:1354-1364
关键词Solar Chromosphere Magnetic Field Velocity Field
ISSN号1001-6511
通讯作者HU, WR (reprint author), ACAD SINICA,INST MECH,BEIJING 100080,PEOPLES R CHINA.
中文摘要The data of velocity and magnetic fields in the solar photosphere (5324 angstrom) and the chromosphere (4861 angstrom) clearly show the features of tangential discontinuity of velocity in the chromosphere. The velocity fields in and near the solar active region named No. 88029 by the Huairou Station have been analyzed in detail. A lot of magnetohydrodynamic discontinuous surfaces, especially the tangential discontinuities, are shown from the observations. The calculations of the thickness of discontinuous layer and the evolution time of instability agree with the observational results. The variations of the flow field will directly influence the evolutions and changes of the active region as the magnetic field are coupled closely with the plasma motion.
类目[WOS]Mathematics, Applied ; Mathematics
研究领域[WOS]Mathematics
收录类别SCI
语种英语
WOS记录号WOS:A1991GY89600009
公开日期2009-08-03 ; 2010-08-20
源URL[http://dspace.imech.ac.cn/handle/311007/39500]  
专题力学研究所_力学所知识产出(1956-2008)
推荐引用方式
GB/T 7714
Hu WR,Zhang HQ,Chen JM. The tangential discontinuous surface of velocity in solar chromosphere[J]. Science in China Series A-Mathematics Physics Astronomy,1991,34(11):1354-1364.
APA 胡文瑞,Zhang HQ,&Chen JM.(1991).The tangential discontinuous surface of velocity in solar chromosphere.Science in China Series A-Mathematics Physics Astronomy,34(11),1354-1364.
MLA 胡文瑞,et al."The tangential discontinuous surface of velocity in solar chromosphere".Science in China Series A-Mathematics Physics Astronomy 34.11(1991):1354-1364.

入库方式: OAI收割

来源:力学研究所

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