论文标题

动力学alfvén波和热电子之间的非线性兰道谐振相互作用:时域结构的激发

Nonlinear Landau resonant interaction between kinetic Alfvén waves and thermal electrons: Excitation of time domain structures

论文作者

An, Xin, Bortnik, Jacob, Zhang, Xiaojia

论文摘要

相位空间孔,双层和其他孤立电场结构,称为时域结构(TDSS),通常发生在地球内部磁层中的偶极性前方周围。它们被认为很重要,因为它们在注入能量的耗散中的作用及其在明显的颗粒散射和加速度的潜力中的作用。观察到动力学的alfvén波在能量颗粒注射过程中受到激发,通常与TDS观测值一起存在。尽管有大量的航天器观测值,但迄今为止,TDSS的起源及其与动力学alfvén波的关系仍然很众所周知。一部分难度源于动力学alfvén波和TDS之间的巨大分离。在这里,我们证明了与动力学alfvén波的非线性Landau共鸣中的电子可以激发TDS。这些电子被动力学alfvén波的平行电场捕获,形成局部束分布,然后通过梁的不稳定性生成TDS。大图的出现如下:宏观偶极化前端首先将离子流(动力学)能量转移到中等尺度的动力学alfvén波中,这进一步将能量进一步将能量传递给微观的TDS,并最终以加热形式将能量沉积到热电子中。这样,与偶极化前端相关的离子流能有效地消散在从内部磁层中的大到小尺度的级联反应中。

Phase space holes, double layers and other solitary electric field structures, referred to as time domain structures (TDSs), often occur around dipolarization fronts in the Earth's inner magnetosphere. They are considered to be important because of their role in the dissipation of the injection energy and their potential for significant particle scattering and acceleration. Kinetic Alfvén waves are observed to be excited during energetic particle injections, and are typically present in conjunction with TDS observations. Despite the availability of a large number of spacecraft observations, the origin of TDSs and their relation to kinetic Alfvén waves remains poorly understood to date. Part of the difficulty arises from the vast scale separations between kinetic Alfvén waves and TDSs. Here, we demonstrate that TDSs can be excited by electrons in nonlinear Landau resonance with kinetic Alfvén waves. These electrons get trapped by the parallel electric field of kinetic Alfvén waves, form localized beam distributions, and subsequently generate TDSs through beam instabilities. A big picture emerges as follows: macroscale dipolarization fronts first transfer the ion flow (kinetic) energy to kinetic Alfvén waves at intermediate scale, which further channel the energy to TDSs at the microscale and eventually deposit the energy to the thermal electrons in the form of heating. In this way, the ion flow energy associated with dipolarization fronts is effectively dissipated in a cascade from large to small scales in the inner magnetosphere.

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