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Nonlinear Waves in Collisional Ionospheric Plasmas

机译:碰撞电离层等离子体中的非线性波

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摘要

A unified electrostatic MHD theory is developed to describe small-scale plasma structures with arbitrary amplitude moving in auroral ionosphere, or magnetosphere, with a constant velocity V in respect to ambient plasma, which is drifting under the action of large-scale electric field E. The theoretical model includes additional dissipative terms in comparison with that described in accompanying paper by the same authors. It accounts for ion and electron inertia, dynamic ion viscosity, deviation from quasi-neutrality. The equations are derived in respect to the variable S = x - Vt for one-dimensional models, and S = x + αz - Vt for a two-dimensional model. In the two-dimensional form of the theory for the strongly collisional case, the vector nonlinearity (or, Poisson brackets) gives the main stabilizing effect to the two-stream instability leading to a stationary turbulence level with density fluctuations of order 10% or more. Damped large-amplitude oscillations superimposed on an electrostatic shock are excited which can be VHF radar aurora scatterers for the non-zero aspect angles. Qualitative agreement with the results of radar aurora studies and in situ rocket measurements is found.
机译:发展了统一的静电MHD理论,以描述在极光电离层或磁层中以任意幅度移动,相对于周围等离子体具有恒定速度V的小规模等离子体结构,该结构在大电场E的作用下漂移。与同一作者在随附论文中描述的模型相比,该理论模型还包含其他耗散术语。它考虑了离子和电子惯性,动态离子粘度,与准中性的偏差。对于一维模型,关于变量S = x-Vt推导方程;对于二维模型,关于S = x +αz-Vt推导方程。在强碰撞情况下的二维理论形式中,矢量非线性(或泊松括号)为两流不稳定性提供了主要的稳定作用,从而导致了密度波动为10%或更大的平稳湍流能级。叠加在静电冲击上的阻尼大振幅振荡被激发,这可能是VHF雷达极光散射体(对于非零长宽角)。发现与雷达极光研究和现场火箭测量的结果在质量上吻合。

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