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Generalized Bohm sheath criterion in dusty plasma of space environment
Advances in Space Research ( IF 2.8 ) Pub Date : 2021-07-01 , DOI: 10.1016/j.asr.2021.06.020
S. Davood Sadatian , M. Gharjeh ghiyaei

By introducing the Kappa distribution function (κ) and considering the dimensionless variables and applying them to the Poisson equation, the Bohm sheath equation in a plasma is obtained. We know the above distribution function has two important factors: 1-the invariant kappa spectral index (κ0), 2-the number of degrees of freedom (de,Φ). In this regard, we considered soliton with positive and negative potentials in the two areas of the solar structure Heliosphere (positive potential: near equilibrium areas κ0>1 and negative potential Heliosheath: out of equilibrium areas 0<κ0<1). Then, the Korteweg-de-Vries equation (KdV) is obtained using the Bohm criterion and applying the Sagdeev pseudo potential method and effects of the spectral index κ0, the potential degrees of freedom de,Φ via perturbation are studied numerically.



中文翻译:

空间环境尘埃等离子体中的广义玻姆鞘判据

通过引入 Kappa 分布函数(κ) 并考虑无量纲变量并将它们应用于泊松方程,得到等离子体中的玻姆鞘方程。我们知道上面的分布函数有两个重要的因素:1-不变的kappa谱指数(κ0), 2-自由度数 (d电子,Φ)。在这方面,我们考虑了太阳结构日光层两个区域中具有正负电位的孤子(正电位:接近平衡区域κ0>1 和负电位 Heliosheath:超出平衡区域 0<κ0<1)。然后,使用 Bohm 准则并应用 Sagdeev 伪电位方法和光谱指数的影响,获得 Korteweg-de-Vries 方程 (KdV)κ0, 潜在的自由度 d电子,Φ 通过扰动进行数值研究。

更新日期:2021-08-24
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