地球磁层中自引力碰撞磁化尘埃等离子体中非线性尘埃声波的传播

IF 1.6 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
A. Almuqrin, M. Alotiby, R. Tolba
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引用次数: 0

摘要

研究了在由带负电荷的尘埃粒子、麦克斯韦电子和离子组成的磁化尘埃等离子体中,不同类型的DANW声尘埃非线性波的非线性传播。应用标准归约微扰理论推导了相应的三维非线性复Ginzburg–Landau(3D-CGLE)方程,该方程控制了尘埃声波包的动力学。数值分析了CGLE的稳态解析解,其中考虑了尘埃等离子体模型的物理参数对波传播的影响。研究发现,孤立波的出现与电磁波之间,以及类冲击波与周期行波之间可能存在关系。表达这些发现的重要性是解释空间物理学中非线性波传播之间真实关系的基石,例如地球磁场。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Propagation of Nonlinear Dust-Acoustic Waves in a Self-Gravitating Collision Magnetized Dusty Plasma in Earth’s Magnetosphere
The nonlinear propagation of different types of DANW acoustic dust nonlinear waves has been investigated in a magnetized dusty plasma consisting of negatively charged dust particles, Maxwellian electrons, and ions. Application of the standard reductive perturbation theory is used to derive the corresponding three-dimensional nonlinear a complex Ginzburg–Landau (3D-CGLE) equation which governs the dynamics of the dust-acoustic wave packets. The stationary analytical solutions of the CGLE are numerically analysed where the effect of the physical parameters of the dusty plasma model on the wave’s propagation is taken into account. It has been found that there can be a relationship between the appearance of soliton waves and electromagnetic waves, as well as between shock-like waves and periodic travelling waves. Expression of the importance of these findings is the cornerstone of explaining the true relationship between the propagation of nonlinear waves in the physics of space, for example, the Earth’s magnetic field.
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来源期刊
Advances in Astronomy
Advances in Astronomy ASTRONOMY & ASTROPHYSICS-
CiteScore
2.70
自引率
7.10%
发文量
10
审稿时长
22 weeks
期刊介绍: Advances in Astronomy publishes articles in all areas of astronomy, astrophysics, and cosmology. The journal accepts both observational and theoretical investigations into celestial objects and the wider universe, as well as the reports of new methods and instrumentation for their study.
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