Dynamical characteristics of a higher dimensional model of magnetized Rossby waves in the ionospheric E-layer and modulational instability analysis

IF 1.9 4区 物理与天体物理 Q3 PHYSICS, CONDENSED MATTER
Yanshang Li, Xiaojun Yin, Ruigang Zhang, Quansheng Liu
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Abstract

Rossby waves are important large-scale dynamic wave modes in geophysical fluids. In the ionospheric E-region, magnetized Rossby waves significantly modulate plasma motion through nonlinear coupling with neutral winds and the dynamo process. Thus, they play an important role in the evolution of ionospheric dynamics. This study focuses on the nonlinear dynamic characteristics of magnetized Rossby waves. Using the geomagnetically corrected quasi-geostrophic potential vorticity theory, multi-scale perturbation expansion, and coordinate transformation, we derive the (2+1)-dimensional Kadomtsev–Petviashvili (KP) equation. The Hirota bilinear method is used to solve this equation, obtaining breather-type traveling wave solutions. Rogue wave solutions are further constructed via the homoclinic breather limit method. Modulational instability analysis confirms that the real constant background steady-state solution is linearly stable. Numerical simulations are performed to plot amplitude evolution, two-dimensional distributions, and flow field evolutions of the solutions under different background flows. The influences of the \(\beta \) effect and the geomagnetic latitudinal gradient effect on the flow field evolution of the two solutions are also investigated. Results show that breather-type traveling waves have stable periodic oscillation and directional propagation. Rogue waves exhibit obvious spatiotemporal localization, with sudden amplitude amplification and rapid attenuation. Variations in the \(\beta \) effect and geomagnetic latitudinal gradient effect trigger changes in the generalized Rossby parameter, which substantially modulates the evolution of the two types of wave motions. This study clarifies the nonlinear propagation laws and coherent structure characteristics of magnetized Rossby waves, providing important theoretical support for ionospheric wave dynamics research and space weather prediction.

电离层e层磁化罗斯比波高维模型的动力学特性及调制不稳定性分析
罗斯比波是地球物理流体中重要的大尺度动力波。在电离层e区,磁化罗斯比波通过与中性风和发电机过程的非线性耦合显著调节等离子体运动。因此,它们在电离层动力学的演化中起着重要的作用。本文主要研究磁化罗斯比波的非线性动力学特性。利用地磁校正准地转位涡理论、多尺度微扰展开和坐标变换,导出了(2+1)维Kadomtsev-Petviashvili (KP)方程。利用Hirota双线性方法求解该方程,得到呼吸型行波解。利用同斜呼吸极限法进一步构造了异常波解。调制不稳定性分析证实了实际恒定背景稳态解是线性稳定的。通过数值模拟,绘制了不同背景流下解的幅值演化、二维分布和流场演化。研究了\(\beta \)效应和地磁纬向梯度效应对两种解流场演化的影响。结果表明,呼吸型行波具有稳定的周期振荡和定向传播。异常波具有明显的时空局域性,振幅放大突然,衰减迅速。\(\beta \)效应和地磁纬向梯度效应的变化引发广义Rossby参数的变化,而广义Rossby参数的变化实质上调节了两种波的演化。本研究阐明了磁化罗斯比波的非线性传播规律和相干结构特征,为电离层波动力学研究和空间天气预报提供了重要的理论支持。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
The European Physical Journal B
The European Physical Journal B 物理-物理:凝聚态物理
CiteScore
2.80
自引率
6.20%
发文量
184
审稿时长
5.1 months
期刊介绍: Solid State and Materials; Mesoscopic and Nanoscale Systems; Computational Methods; Statistical and Nonlinear Physics
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