金星低层电离层中的非线性离子声波动力学

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Kusum Chettri, Jharna Tamang, Prasanta Chatterjee, Asit Saha
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引用次数: 0

摘要

研究了金星低层大气中高度为(200-1000)千米的非线性离子声波(IAWs)的动力学。研究了由\(H^{+}\)和\(O^{+}\)离子与卡帕分布电子组成的三分量等离子体中的双孤立子、非线性孤波和周期波。利用还原扰动技术(RPT)推导出了 Korteweg-de Vries(KdV)方程,并利用行波变换为 KdV 方程建立了平面动力系统。通过调整参数 \(\kappa\)(频谱指数)、\(\gamma\)(未扰动数密度比)和\(V\)(行波速度),绘制出相位肖像来分析非线性波行为。kappa)值的增加会放大孤波和周期波的振幅,缩小孤波的宽度,扩大周期波的宽度。gamma)值的增加会增强孤波的振幅,宽度不变,而非线性周期波的振幅减小,宽度变宽。增加(V)值会增强孤波和周期波的振幅并减小宽度。使用 Hirota 直接法研究了 KdV 方程的双孤子解。伽马值的增加会减小孤子的振幅而不影响宽度,卡帕值的增加会减小孤子的宽度。我们还显示了双孤子的相移,发现对于不同的\(\kappa \)值,相移随着\(\gamma \)值的增加而增加。我们的研究结果有助于理解金星低电离层中非线性波和双oliton解的动力学。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Dynamics of nonlinear ion-acoustic waves in Venus’ lower ionosphere

Dynamics of nonlinear ion-acoustic waves in Venus’ lower ionosphere

Dynamics of nonlinear ion-acoustic waves (IAWs) are studied for Venus’ lower atmosphere at an altitude of \(200-1000\) km. Two-soliton, nonlinear solitary and periodic waves in a three-component plasma consisting of \(H^{+}\) and \(O^{+}\) ions with kappa distributed electrons are studied. Using the reductive perturbation technique (RPT), the Korteweg-de Vries (KdV) equation is derived and a Planar dynamical system is formed for the KdV equation using a travelling wave transformation. A phase portrait is drawn to analyze nonlinear wave behaviors by adjusting the parameters \(\kappa \) (spectral index), \(\gamma \) (unperturbed number density ratio), and \(V\) (travelling wave speed). Increasing values of \(\kappa \) amplify amplitudes for solitary and periodic waves, narrow down the width of the solitary wave, and broaden the width of the periodic wave. Increasing value of \(\gamma \) boosts amplitude of the solitary wave with unchanged width, while amplitude of the nonlinear periodic wave decreases and width widens. Increasing value of \(V\) enhances amplitudes and reduces widths for both solitary and periodic waves. Two-soliton solutions for the KdV equation are studied using the Hirota direct method. Increasing value of \(\gamma \) reduces amplitude of the soliton without affecting the width and increasing value of \(\kappa \) reduces width of the soliton. Phase shift for two-soliton is also shown and found that for different values of \(\kappa \), the phase shift increases on increasing value of \(\gamma \). The findings of our result aid in understanding the dynamics of nonlinear waves and two-soliton solutions in Venus’ lower ionosphere.

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来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
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