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首页> 外文期刊>Physics of plasmas >Study of electric and magnetic field fluctuations from lower hybrid drift instability waves in the terrestrial magnetotail with the fully kinetic, semi-implicit, adaptive multi level multi domain method
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Study of electric and magnetic field fluctuations from lower hybrid drift instability waves in the terrestrial magnetotail with the fully kinetic, semi-implicit, adaptive multi level multi domain method

机译:用全动力学,半隐式,自适应多级多域方法研究地面磁尾中较低混合漂移不稳定波的电场和磁场波动

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摘要

The newly developed fully kinetic, semi-implicit, adaptive multi-level multi-domain (MLMD) method is used to simulate, at realistic mass ratio, the development of the lower hybrid drift instability (LHDI) in the terrestrial magnetotail over a large wavenumber range and at a low computational cost. The power spectra of the perpendicular electric field and of the fluctuations of the parallel magnetic field are studied at wavenumbers and times that allow to appreciate the onset of the electrostatic and electromagnetic LHDI branches and of the kink instability. The coupling between electric and magnetic field fluctuations observed by Norgren et al. ["Lower hybrid drift waves: Space observations," Phys. Rev. Lett. 109, 055001 (2012)] for high wavenumber LHDI waves in the terrestrial magnetotail is verified. In the MLMD simulations presented, a domain ("coarse grid") is simulated with low resolution. A small fraction of the entire domain is then simulated with higher resolution also ("refined grid") to capture smaller scale, higher frequency processes. Initially, the MLMD method is validated for LHDI simulations. MLMD simulations with different levels of grid refinement are validated against the standard semi-implicit particle in cell simulations of domains corresponding to both the coarse and the refined grid. Precious information regarding the applicability of the MLMD method to turbulence simulations is derived. The power spectra of MLMD simulations done with different levels of refinements are then compared. They consistently show a break in the magnetic field spectra at k(perpendicular to)d(i) similar to 30, with d(i) the ion skin depth and k(perpendicular to) the perpendicular wavenumber. The break is observed at early simulated times, Omega(ci)t < 6, with Omega(ci) the ion cyclotron frequency. It is due to the initial decoupling of electric and magnetic field fluctuations at intermediate and low wavenumbers, before the development of the electromagnetic LHDI branch. Evidence of coupling between electric and magnetic field fluctuations in the wave-number range where the fast and slow LHDI branches develop is then provided for a cluster magnetotail crossing. Published by AIP Publishing.
机译:新开发的全动力学,半隐式,自适应多级多域(MLMD)方法用于在实际质量比下模拟大波数下地面磁尾的低混合漂移不稳定性(LHDI)的发展范围和较低的计算成本。在波数和时间上研究了垂直电场的功率谱和平行磁场的波动,可以了解静电和电磁LHDI分支的开始以及纽结的不稳定性。 Norgren等人观察到的电场和磁场波动之间的耦合。 [“低杂波漂移波:空间观测”,物理学。牧师109,055001(2012)]验证了地面磁尾中的高波数LHDI波。在提出的MLMD模拟中,以低分辨率模拟了一个域(“粗网格”)。然后,也以更高的分辨率(“精制网格”)模拟整个域的一小部分,以捕获规模较小,频率较高的过程。最初,MLMD方法已针对LHDI仿真进行了验证。在对应于粗网格和精化网格的域的单元格仿真中,针对标准半隐式粒子对具有不同网格精化级别的MLMD仿真进行了验证。得出有关MLMD方法在湍流模拟中的适用性的宝贵信息。然后比较了在不同细化水平下完成的MLMD仿真的功率谱。它们始终显示出在k(垂直于)d(i)处类似于30的磁场频谱中的断裂,其中d(i)离子趋肤深度和k(垂直于)垂直波数。在早期模拟时间观察到此中断,Omega(ci)t <6,离子回旋加速器频率为Omega(ci)。这是由于在电磁LHDI分支发展之前,中波和低波数处的电场和磁场波动的初始解耦。然后为簇磁尾交叉提供了波数范围内电场和磁场波动之间耦合的证据,快速和慢速LHDI分支在该波数范围内发展。由AIP Publishing发布。

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