离子源项对电负性尘埃等离子体鞘层的影响

IF 2.1 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
S.A. Galyanseyedi , G. Foroutan , T. Mohsenpour
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引用次数: 0

摘要

本研究考察了磁电负性尘埃等离子体鞘的固定模型,将尘埃颗粒视为冷流体。在该模型中,电子和负离子处于麦克斯韦热力学平衡,而正离子被认为是具有离子源项的热流体。离子源和电离频率(if)对鞘的影响进行了检查,比较他们的贡献。利用Sagdeev势法,从理论上建立了改进的鞘层判据和浮动势。然后对模型的控制方程进行了数值求解。研究了离子源对鞘层电位、粒子密度、正离子速度和空间电荷密度的影响。结果表明,修正Bohm准则随IF的增大而减小。可见,不同离子源项在尘埃等离子体鞘层结构中是有效的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Effects of ion source term on the sheath in electronegative dusty plasmas
This study examines a stationary model of the magneto-electronegative dusty plasma sheath, treating dust particles as a cold fluid. In the present model, the electron and negative ion are in Maxwellian thermodynamic equilibrium, while positive ions are considered as a hot fluid with an ion source term. The effects of ion sources and ionization frequencies (IFs) on the sheath are examined to compare their contributions. A modified sheath criterion and floating potential are established theoretically using the Sagdeev potential method. The governing equations of the model are then solved numerically. The effects of the ion source on sheath electric potential, particle density, positive ion velocity, and space charge density are also investigated. It was found that the modified Bohm criterion decreases with an increase of the IF. It can be seen that the different ion source term is effective in the dusty plasma sheath structure.
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来源期刊
New Astronomy
New Astronomy 地学天文-天文与天体物理
CiteScore
4.00
自引率
10.00%
发文量
109
审稿时长
13.6 weeks
期刊介绍: New Astronomy publishes articles in all fields of astronomy and astrophysics, with a particular focus on computational astronomy: mathematical and astronomy techniques and methodology, simulations, modelling and numerical results and computational techniques in instrumentation. New Astronomy includes full length research articles and review articles. The journal covers solar, stellar, galactic and extragalactic astronomy and astrophysics. It reports on original research in all wavelength bands, ranging from radio to gamma-ray.
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