Generation of electromagnetic ion cyclotron waves in the near-Earth magnetotail during dipolarization: Two-dimensional global hybrid simulation

被引:3
|
作者
Guo, Zhifang [1 ,3 ]
Wu, Mingyu [2 ,4 ]
Du, Aimin [1 ]
机构
[1] Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
[2] Univ Sci & Technol China, Dept Geophys & Planetary Sci, CAS Key Lab Geospace Environm, Hefei 230026, Peoples R China
[3] Univ Chinese Acad Sci, Beijing, Peoples R China
[4] Collaborat Innovat Ctr Astronaut Sci & Technol, Harbin, Peoples R China
基金
美国国家科学基金会;
关键词
MAGNETIC PULSATIONS; PLASMA; MAGNETOSPHERE; AMPLIFICATION; INSTABILITY; DIFFUSION; DYNAMICS;
D O I
10.1063/1.4947567
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
We employ two-dimensional global hybrid simulations to study the generation, propagation, and polarization of electromagnetic ion cyclotron (EMIC) waves in the near-Earth magnetotail (around x = -10R(E)) during dipolarization. In our simulation, EMIC waves with left-hand polarized signals originate in the low-latitude magnetotail as a result of the ion temperature anisotropy which is due to ion heating by Alfven waves. Subsequently, EMIC waves can propagate along the ambient magnetic field toward high-latitudes. Our work provides one possible mechanism for the generation of EMIC waves observed in the near-Earth magnetotail. Published by AIP Publishing.
引用
收藏
页数:6
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