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DOI | 10.1029/2019GL082709 |
Thin Current Sheets of Sub-ion Scales observed by MAVEN in the Martian Magnetotail | |
Grigorenko, E. E.1,2; Zelenyi, L. M.1,2; DiBraccio, G.3; Ermakov, V. N.1; Shuvalov, S. D.1; Malova, H. V.1,4; Popov, V. Y.1,4,5; Halekas, J. S.6; Mitchell, D. L.7; Dubinin, E.8 | |
2019-06-28 | |
发表期刊 | GEOPHYSICAL RESEARCH LETTERS
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ISSN | 0094-8276 |
EISSN | 1944-8007 |
出版年 | 2019 |
卷号 | 46期号:12页码:6214-6222 |
文章类型 | Article |
语种 | 英语 |
国家 | Russia; USA; Germany |
英文摘要 | Current sheets (CSs) play a crucial role in the storage and conversion of magnetic energy in planetary magnetotails. Using high-resolution magnetic field data from MAVEN spacecraft, we report the existence of super thin current sheets (STCSs) in the Martian magnetotail. The typical half-thickness of the STCSs is similar to 5 km, and it is much less than the gyroradius of thermal protons (rho(p)). The STCSs are embedded into a thicker sheet with L >= rho(p) forming a multiscale current configuration. The formation of STCS does not depend on ion composition, but it is controlled by the small value of the normal component of the magnetic field at the neutral plane (B-N). A number of the observed multiscale CSs are located in the parametric map close to the tearing-unstable domain, and thus, the inner STCS can provide an additional free energy to excite ion tearing mode in the Martian magnetotail. Plain Language Summary We investigate the structure of cross-tail current sheets (CSs) in the Martian magnetotail. The CSs play a crucial role in the conversion of magnetic energy into kinetic and thermal energy of plasma particles via magnetic reconnection. Signatures of magnetic reconnection were reported in the Martian magnetotail, but the mechanisms leading to reconnection onset are still unknown. Previous observations in the Earth magnetotail showed that the stretching of the CS magnetic configuration leads to formation of thin CS embedded into a thicker one. Such multiscale configuration can be a source of free energy for excitation of ion tearing mode. The development of this mode can generate X-type and/or O-type magnetic configuration and trigger reconnection. By using MAVEN spacecraft observations, we reported the formation of multiscale CS structure in the Martian magnetotail with the inner super thin current sheet (STCS) having a half-thickness much less than proton gyroradius. We showed that the STCS can be in the metastable state. Thus, the CS thinning and the formation of STCS can lead to a new metastable equilibrium, in which the CS undergoes topological changes enabling the process of fast magnetic reconnection. |
英文关键词 | Martian magnetotail Current Sheet |
领域 | 气候变化 |
收录类别 | SCI-E |
WOS记录号 | WOS:000477616300007 |
WOS关键词 | TAIL CURRENT SHEET ; MAGNETIC-FIELD ; MARS ; PLASMA ; RECONNECTION ; CONFIGURATION ; BODIES ; WAKES |
WOS类目 | Geosciences, Multidisciplinary |
WOS研究方向 | Geology |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://119.78.100.173/C666/handle/2XK7JSWQ/184206 |
专题 | 气候变化 |
作者单位 | 1.RAS, Space Res Inst, Moscow, Russia; 2.Moscow Inst Phys & Technol, Moscow, Russia; 3.NASA, Goddard Space Flight Ctr, Greenbelt, MD USA; 4.Moscow MV Lomonosov State Univ, Dept Phys, Moscow, Russia; 5.Natl Univ, Higher Sch Econ, Moscow, Russia; 6.Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA; 7.Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA; 8.Max Planck Inst Solar Syst Res, Gottingen, Germany |
推荐引用方式 GB/T 7714 | Grigorenko, E. E.,Zelenyi, L. M.,DiBraccio, G.,et al. Thin Current Sheets of Sub-ion Scales observed by MAVEN in the Martian Magnetotail[J]. GEOPHYSICAL RESEARCH LETTERS,2019,46(12):6214-6222. |
APA | Grigorenko, E. E..,Zelenyi, L. M..,DiBraccio, G..,Ermakov, V. N..,Shuvalov, S. D..,...&Dubinin, E..(2019).Thin Current Sheets of Sub-ion Scales observed by MAVEN in the Martian Magnetotail.GEOPHYSICAL RESEARCH LETTERS,46(12),6214-6222. |
MLA | Grigorenko, E. E.,et al."Thin Current Sheets of Sub-ion Scales observed by MAVEN in the Martian Magnetotail".GEOPHYSICAL RESEARCH LETTERS 46.12(2019):6214-6222. |
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