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Magnetic Reconnection in the Near Venusian Magnetotail

文献类型：期刊论文

作者Zhang, T. L.1,2; Lu, Q. M.1; Baumjohann, W.2; Russell, C. T.3; Fedorov, A.4; Barabash, S.5; Coates, A. J.6; Du, A. M.7; Cao, J. B.8; Nakamura, R.2
刊名SCIENCE
出版日期2012-05-04
卷号336期号:6081页码:567-570
ISSN号0036-8075
DOI10.1126/science.1217013
文献子类Article
英文摘要Observations with the Venus Express magnetometer and low-energy particle detector revealed magnetic field and plasma behavior in the near-Venus wake that is symptomatic of magnetic reconnection, a process that occurs in Earth's magnetotail but is not expected in the magnetotail of a nonmagnetized planet such as Venus. On 15 May 2006, the plasma flow in this region was toward the planet, and the magnetic field component transverse to the flow was reversed. Magnetic reconnection is a plasma process that changes the topology of the magnetic field and results in energy exchange between the magnetic field and the plasma. Thus, the energetics of the Venus magnetotail resembles that of the terrestrial tail, where energy is stored and later released from the magnetic field to the plasma.
WOS关键词TAIL RECONNECTION ; FLUX ROPES ; ATMOSPHERE ; EXPRESS
WOS研究方向Science & Technology - Other Topics
语种英语
WOS记录号WOS:000303498800040
出版者AMER ASSOC ADVANCEMENT SCIENCE
资助机构National Natural Science Foundation of China(41121003 ; National Natural Science Foundation of China(41121003 ; Austrian Science Fund(FWF: I429-N16) ; Austrian Science Fund(FWF: I429-N16) ; NASA(NNX10AV29G) ; NASA(NNX10AV29G) ; 41174156) ; 41174156) ; National Natural Science Foundation of China(41121003 ; National Natural Science Foundation of China(41121003 ; Austrian Science Fund(FWF: I429-N16) ; Austrian Science Fund(FWF: I429-N16) ; NASA(NNX10AV29G) ; NASA(NNX10AV29G) ; 41174156) ; 41174156) ; National Natural Science Foundation of China(41121003 ; National Natural Science Foundation of China(41121003 ; Austrian Science Fund(FWF: I429-N16) ; Austrian Science Fund(FWF: I429-N16) ; NASA(NNX10AV29G) ; NASA(NNX10AV29G) ; 41174156) ; 41174156) ; National Natural Science Foundation of China(41121003 ; National Natural Science Foundation of China(41121003 ; Austrian Science Fund(FWF: I429-N16) ; Austrian Science Fund(FWF: I429-N16) ; NASA(NNX10AV29G) ; NASA(NNX10AV29G) ; 41174156) ; 41174156)
源URL[http://ir.iggcas.ac.cn/handle/132A11/84170]  
专题中国科学院地质与地球物理研究所
通讯作者Zhang, T. L.
作者单位1.Univ Sci & Technol China, Chinese Acad Sci, Key Lab Geospace Environm, Hefei 230026, Peoples R China
2.Austrian Acad Sci, Space Res Inst, A-8042 Graz, Austria
3.Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90095 USA
4.Ctr Etud Spatiale Rayonnements, F-31028 Toulouse, France
5.Swedish Inst Space Phys, S-98128 Kiruna, Sweden
6.Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
7.Chinese Acad Sci, Inst Geol & Geophys, Beijing 100029, Peoples R China
8.Beihang Univ, Space Sci Inst, Beijing 100191, Peoples R China
9.Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, D-38106 Braunschweig, Germany
10.Univ Sheffield, Dept Automat Control & Syst Engn, Sheffield S1 3JD, S Yorkshire, England
推荐引用方式
GB/T 7714		 Zhang, T. L.,Lu, Q. M.,Baumjohann, W.,et al. Magnetic Reconnection in the Near Venusian Magnetotail[J]. SCIENCE,2012,336(6081):567-570.
APA Zhang, T. L..,Lu, Q. M..,Baumjohann, W..,Russell, C. T..,Fedorov, A..,...&Balikhin, M..(2012).Magnetic Reconnection in the Near Venusian Magnetotail.SCIENCE,336(6081),567-570.
MLA Zhang, T. L.,et al."Magnetic Reconnection in the Near Venusian Magnetotail".SCIENCE 336.6081(2012):567-570.

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来源：地质与地球物理研究所

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