Numerical study of magnetic reconnection possibly occurring near heliospheric current sheet | |
Wei, F. S.; Feng, X. S.; Hu, Q.; 北京8701信箱 | |
Department | 空间天气学国家重点实验室 |
Source Publication | Space Weather
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2005 | |
Volume | 36Issue:12Pages:2303-2307 |
ISSN | 0273-1177 |
Language | 英语 |
Keyword | Magnetic Reconnection Numerical Study Heliospheric Current Sheet Space Plasma Interplanetary Magnetosphere |
Abstract | The third-order accurate upwind compact difference scheme has been applied for the numerical study of the magnetic reconnection driven by a plasma blob impacting the heliospheric current sheet, under the framework of the two-dimensional compressible magnetohydrodynamics. The results show that the driven reconnection near the current sheet could occur in about 10-30 min for the interplanetary high magnetic Reynolds number, R-M = 2000-10,000, a stable magnetic reconnection structure can be formed in hour order of magnitude, and there appear some basic properties such as the multiple X-line reconnections, vortex structures, filament current systems, splitting and collapse of the high-density plasma blob. These results are helpful in understanding and identifying the magnetic reconnection phenomena possibly occurring near the heliospheric current sheets. |
Indexed By | SCI |
Funding Project | 中国科学院空间科学与应用研究中心 |
Document Type | 期刊论文 |
Identifier | http://ir.nssc.ac.cn/handle/122/1037 |
Collection | 空间科学部 |
Corresponding Author | 北京8701信箱 |
Recommended Citation GB/T 7714 | Wei, F. S.,Feng, X. S.,Hu, Q.,et al. Numerical study of magnetic reconnection possibly occurring near heliospheric current sheet[J]. Space Weather,2005,36(12):2303-2307. |
APA | Wei, F. S.,Feng, X. S.,Hu, Q.,&北京8701信箱.(2005).Numerical study of magnetic reconnection possibly occurring near heliospheric current sheet.Space Weather,36(12),2303-2307. |
MLA | Wei, F. S.,et al."Numerical study of magnetic reconnection possibly occurring near heliospheric current sheet".Space Weather 36.12(2005):2303-2307. |
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