The Induced Magnetosphere of Mars: Asymmetrical Topology of the Magnetic Field Lines
文献类型：期刊论文
| 作者 | Dubinin, E.6; Modolo, R.7; Fraenz, M.6; Paeetzold, M.3; Woch, J.6; Chai, L.4; Wee, Y.4; Connerney, J. E. P.2; Mcfadden, J.5; DiBraccio, G.2 |
| 刊名 | GEOPHYSICAL RESEARCH LETTERS
 |
| 出版日期 | 2019-11-28 |
| 卷号 | 46期号:22页码:12722-12730 |
| ISSN号 | 0094-8276 |
| DOI | 10.1029/2019GL084387 |
| 英文摘要 | An asymmetrical pileup of the interplanetary magnetic field leads to an additional draping of the field lines in the opposite direction to the motional electric field. Such a draping and the associated magnetic field forces push the ionosphere plasma in the transverse direction opening a passage for an ion trail which contains dense and slowly moving plasma. We found that wrapping of the field lines around Mars starts in the hemisphere pointing in the direction of the motional electric field and propagates to the opposite hemisphere where the cross-flow component of the draped interplanetary magnetic field changes sign in a broad area accompanied by the formation of loops of closed field lines. Reconnection near Mars accompanied by the generation of plasma vortices imposes serious constraints on the ion dynamics and their escape through the tail. The existence of all these features is confirmed by hybrid simulations. |
| WOS关键词 | MARTIAN MAGNETOTAIL ; MAVEN ; RECONNECTION ; MORPHOLOGY ; ESCAPE ; PLASMA |
| 资助项目 | NASA ; DFG[PA 525/14-1] ; DLR[50QM1703] |
| WOS研究方向 | Geology |
| 语种 | 英语 |
| 出版者 | AMER GEOPHYSICAL UNION |
| WOS记录号 | WOS:000505879600009 |
| 资助机构 | NASA ; NASA ; DFG ; DFG ; DLR ; DLR ; NASA ; NASA ; DFG ; DFG ; DLR ; DLR ; NASA ; NASA ; DFG ; DFG ; DLR ; DLR ; NASA ; NASA ; DFG ; DFG ; DLR ; DLR |
| 源URL | [http://ir.iggcas.ac.cn/handle/132A11/95916]  |
| 专题 | 地质与地球物理研究所_中国科学院地球与行星物理重点实验室 |
| 通讯作者 | Dubinin, E. |
| 作者单位 | 1.Inst Space Res, Moscow, Russia 2.NASA, Goddard Space Flight Ctr, Greenbelt, MD USA 3.Rhein Inst Umweltforsch, Abt Planetforsch, Cologne, Germany 4.Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China 5.Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA 6.Max Planck Inst Solar Syst Res, Gottingen, Germany 7.UPMC Univ Paris, CNRS, UVSQ Univ, LATMOS IPSL,Paris Saclay, Guyancourt, France |
| 推荐引用方式 GB/T 7714 | Dubinin, E.,Modolo, R.,Fraenz, M.,et al. The Induced Magnetosphere of Mars: Asymmetrical Topology of the Magnetic Field Lines[J]. GEOPHYSICAL RESEARCH LETTERS,2019,46(22):12722-12730. |
| APA | Dubinin, E..,Modolo, R..,Fraenz, M..,Paeetzold, M..,Woch, J..,...&Zelenyi, L..(2019).The Induced Magnetosphere of Mars: Asymmetrical Topology of the Magnetic Field Lines.GEOPHYSICAL RESEARCH LETTERS,46(22),12722-12730. |
| MLA | Dubinin, E.,et al."The Induced Magnetosphere of Mars: Asymmetrical Topology of the Magnetic Field Lines".GEOPHYSICAL RESEARCH LETTERS 46.22(2019):12722-12730. |
入库方式： OAI收割
来源：地质与地球物理研究所
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