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Dust-acoustic solitary waves in a magnetized dusty plasma with nonthermal electrons and trapped ions

机译:磁化尘埃等离子体中的尘埃孤立波   非热电子和被捕获的离子

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摘要

The nonlinear propagation of electrostatic dust-acoustic (DA) waves in amagnetized dusty plasma consisting of negatively charged mobile dusts,nonthermal fast electrons and trapped ions with vortex-like distribution isstudied. Using the reductive perturbation technique, a Korteweg-de Vries(KdV)-like equation is derived which governs the dynamics of thesmall-amplitude solitary waves in a magnetized dusty nonthermal plasma. It isfound that due to the dust thermal pressure, there exists a critical value$(\beta_c)$ of the nothermal parameter $\beta~(>1)$, denoting the percentage ofenergetic electrons, below which the DA solitary waves cease to propagate. Thesoliton solution (travelling wave) of the KdV-like equation is obtained, and isshown to be only of the rarefactive type. The properties of the solitons areanalyzed numerically with the system parameters. It is also seen that theeffect of the static magnetic field (which only modifies the soliton width)becomes significant when the dust gyrofrequency is smaller than one-tenth ofthe dust plasma frequency. Furthermore, the amplitude of the soliton is foundto increase (decrease) when the ratio of the free to trapped ion temperatures$(\sigma)$ is positive (negative). The effects of the system parametersincluding the obliqueness of propagation $(l_z)$ and $\sigma$ on the dynamicsof the DA solitons are also discussed numerically, and it is found that thesoliton structures can withstand perturbations and turbulence during aconsiderable time. The results should be useful for understanding the nonlinearpropagation of DA solitary waves in laboratory and space plasmas (e.g., Earth'smagnetosphere, auroral region, heliospheric environments etc.).
机译:研究了静电尘埃声波在磁化尘埃等离子体中的非线性传播,该等离子体由带负电的流动尘埃,非热快电子和涡旋状分布的俘获离子组成。使用还原摄动技术,推导了类似Korteweg-de Vries(KdV)的方程,该方程控制着磁化的尘埃非热等离子体中小振幅孤波的动力学。发现由于尘埃的热压力,存在一个非热参数$ \ beta〜(> 1)$的临界值$(\ beta_c)$,表示高能电子的百分比,低于该值,DA孤立波停止传播。 。得到了类KdV方程的孤子解(行波),并且显示为稀疏型。孤子的性质通过系统参数进行数值分析。还可以看到,当粉尘回旋频率小于粉尘等离子体频率的十分之一时,静磁场的影响(仅改变孤子宽度)会变得很明显。此外,当自由离子与捕获离子的温度之比为正(负)时,孤子的振幅增加(减小)。还数值讨论了系统参数(包括传播斜率$(l_z)$和$ \ sigma $)对DA孤子动力学的影响,发现孤子结构可以在相当长的时间内承受扰动和湍流。该结果对于理解DA孤波在实验室和空间等离子体(例如地球磁层,极光区域,日光层环境等)中的非线性传播很有用。

著录项

  • 作者

    Misra, A. P.; Wang, Y.;

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  • 年度 2014
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  • 原文格式 PDF
  • 正文语种 {"code":"en","name":"English","id":9}
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