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首页> 外文期刊>Astrophysics and space science >Formation of obliquely propagating dust-ion-acoustic shock waves due to dust charge fluctuation in magnetized nonthermal dusty plasma
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Formation of obliquely propagating dust-ion-acoustic shock waves due to dust charge fluctuation in magnetized nonthermal dusty plasma

机译:磁化非热粉尘等离子体中粉尘电荷波动引起的粉尘离子声斜波传播

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摘要

A theoretical investigation is made on the formation as well as basic properties of dust-ion-acoustic (DIA) shock waves in a magnetized nonthermal dusty plasma consisting of immobile charge fluctuating dust, inertial ion fluid and nonthermal electrons. The reductive perturbation method is employed to derive the Korteweg-de Vries- Burgers equation governing the DIA shock waves. The combined effects of external static magnetic field, obliqueness, nonthermal electron distribution and dust charge fluctuation on the DIA shock waves are also investigated. It is shown that the dust charge fluctuation is a source of dissipation, and is responsible for the formation of the DIA shock waves. It is also observed that the combined effects of obliqueness, nonthermal electron distribution and dust charge fluctuation significantly modify the basic properties of the DIA shock waves. The implications of our results in space and laboratory dusty plasma situations are briefly discussed.
机译:对磁化非热尘埃等离子体中的尘埃离子声波(DIA)冲击波的形成及其基本性质进行了理论研究,该等离子体由固定电荷波动的尘埃,惯性离子流体和非热电子组成。采用还原摄动法来推导控制DIA冲击波的Korteweg-de Vries-Burgers方程。还研究了外部静磁场,倾斜度,非热电子分布和粉尘电荷波动对DIA冲击波的综合影响。结果表明,粉尘电荷的波动是耗散的原因,并且是DIA冲击波形成的原因。还观察到,倾斜,非热电子分布和粉尘电荷波动的综合作用显着改变了DIA冲击波的基本特性。简要讨论了我们的研究结果在太空和实验室尘土飞扬的等离子体环境中的意义。

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