GSTDTAP  > 气候变化
DOI10.1029/2019GL082709
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
ISSN0094-8276
EISSN1944-8007
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
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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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