低杂化漂移波的性质及磁重联电子扩散区附近和内部的能量传递

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Narges Ahmadi, Hantao Ji, Jongsoo Yoo, Robert Ergun, Izzy Thomas, Rahul Banka, Emma Schultz-Stachnik, Alma Alex
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引用次数: 0

摘要

利用磁层多尺度(MMS)任务观测资料,研究了17个磁层顶和9个磁尾重联事件中电子扩散区附近和内部的低混合漂移波(LHDWs)的性质。我们的分析表明,LHDW的类型取决于电子β,随着电子β的增加,LHDW在性质上变得更具电磁性。静电lhdw中从电磁场到粒子的能量传递更高,并且相对于局部磁场在很大程度上是平行的。线性色散分析表明,静电LHDW垂直传播,电磁波斜向传播,归一化波数在0.5 ~ 0.8范围内。对LHDW非线性饱和的简单估计表明,这些波在支持重联电场方面可能起着重要作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Properties of Lower Hybrid Drift Waves and Energy Transfer Near and Inside the Magnetic Reconnection Electron Diffusion Regions

We investigate properties of lower hybrid drift waves (LHDWs) near and inside the electron diffusion regions in 17 magnetopause and 9 magnetotail reconnection events using Magnetospheric MultiScale (MMS) mission observations. Our analysis show that LHDW type depend on the electron beta, as electron beta increases LHDWs become more electromagnetic in nature. The energy transfer from electromagnetic fields to particles is higher in electrostatic LHDWs and it is largely in parallel direction with respect to the local magnetic field. Linear dispersion analysis shows that electrostatic LHDWs are perpendicular propagating while electromagnetic waves propagate in oblique directions and the normalized wavenumber of all LHDW types falls within 0.5–0.8 range. A simple estimate on the LHDW nonlinear saturation suggests a possibly important roles played by these waves in supporting the reconnection electric field.

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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
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