Subion-Scale Flux Rope Nested Inside Ion-Scale Flux Rope in Earth's Magnetotail

被引:4
|
作者
He, R. J. [1 ,2 ]
Fu, H. S. [1 ,2 ]
Liu, Y. Y. [1 ,2 ]
Wang, Z. [1 ,2 ]
Liu, C. M. [1 ,2 ]
机构
[1] Beihang Univ, Sch Space & Environm, Beijing, Peoples R China
[2] Minist Ind & Informat Technol, Key Lab Space Environm Monitoring & Informat Proc, Beijing, Peoples R China
基金
美国国家科学基金会;
关键词
magnetic reconnection; flux rope; cross scale; energy cascade; ROLLING-PIN DISTRIBUTION; ELECTRON ACCELERATION; MAGNETIC RECONNECTION; DIPOLARIZATION FRONTS; TRANSFER EVENTS; DISSIPATION; TOPOLOGY; REGION; SITES;
D O I
10.1029/2021GL096169
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Magnetic flux ropes (MFRs)-transient magnetic structures widely observed in Earth's magnetosphere-play crucial roles in particle acceleration and energy dissipation. MFRs above ion scale have been well studied, while MFRs at subion scales and their coupling with larger-scale ropes still remains not well understood. In this paper, we present the first observation of a subion-scale MFR nested in an ion-scale MFR, using high-resolution data from the magnetospheric multiscale (MMS) mission. We find that the subion-scale MFR hosts more intense plasma activity than the ion-scale MFR, including distinct electron agyrotropy and strong electromagnetic turbulence. In addition, axis of the subion-scale MFR is oblique to that of the ion-scale MFR, indicating that their generation may be ascribed to 3D magnetic reconnection. Observations of such cross-scale structure may shed new lights into understanding energy cascade in space plasmas.
引用
收藏
页数:10
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