The tangential discontinuous surface of velocity in solar chromosphere
文献类型:期刊论文
作者 | Hu WR(胡文瑞)![]() ![]() |
刊名 | Science in China Series A-Mathematics Physics Astronomy
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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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