Two different types of plasmoids in the plasma sheet: Cluster multisatellite analysis application

被引:18
作者
Zhang, Y. C. [1 ]
Shen, C. [1 ]
Liu, Z. X. [1 ]
Rong, Z. J. [2 ,3 ]
Zhang, T. L. [4 ,5 ]
Marchaudon, A. [6 ,7 ]
Zhang, H. [2 ,3 ]
Duan, S. P. [1 ]
Ma, Y. H. [1 ,8 ]
Dunlop, M. W. [9 ]
Yang, Y. Y. [1 ,10 ]
Carr, C. M. [11 ]
Dandouras, I.
机构
[1] Chinese Acad Sci, Ctr Space Sci & Appl Res, State Key Lab Space Weather, Beijing 100190, Peoples R China
[2] Chinese Acad Sci, Inst Geol & Geophys, Key Lab Ionospher Environm, Beijing 100190, Peoples R China
[3] Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing 100190, Peoples R China
[4] Univ Sci & Technol China, Key Lab Basic Plasma Phys, Dept Geophys & Planetary Sci, Hefei 230026, Peoples R China
[5] Austrian Acad Sci, Space Res Inst, A-8010 Graz, Austria
[6] Univ Orleans, Lab Phys & Chim Environm & Espace, Orleans, France
[7] CNRS, F-45071 Orleans, France
[8] Macau Univ Sci & Technol, Space Sci Inst, Taipa, Peoples R China
[9] Rutherford Appleton Lab, Oxford, England
[10] Univ Chinese Acad Sci, Coll Earth Sci, Beijing, Peoples R China
[11] Univ London Imperial Coll Sci Technol & Med, London, England
基金
中国国家自然科学基金;
关键词
Magnetospheric physics; Plasma sheet; Magnetic reconnection; Plasmoid; MAGNETIC-FLUX ROPES; DEEP GEOMAGNETIC TAIL; ENERGETIC ION BURSTS; EARTHS MAGNETOTAIL; GEOTAIL OBSERVATIONS; NEAR-TAIL; FIELD; RECONNECTION; MODELS; LINES;
D O I
10.1002/jgra.50542
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The fine magnetic field structure of two successive plasmoids previously reported is investigated by magnetic rotation analysis using four Cluster satellite data. Between these two plasmoids, opposite trends of curvature radius (R-c) variations of the magnetic field lines from the boundary to the inner part are found. The different variations of R-c reflect that the two plasmoids have different magnetic configurations. The electric current density distributions for both plasmoids are found distinct. The B-y increase and abundant field-aligned currents in the narrow core region of the first plasmoid indicate that a possible magnetic flux rope (MFR) core exists inside. The results indicate that the first observed plasmoid is of a magnetic loop (ML) type (with possible MFR core) and the second plasmoid is of a magnetic flux rope (MFR) type. The coexistence of ML and MFR in the near-Earth plasma sheet may imply that multiple X line reconnection can occur by either an antiparallel or a component-parallel way.
引用
收藏
页码:5437 / 5444
页数:8
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