Nonthermal effects on the cylindrical dusty ion shocks in nonthermal viscous space plasma

被引：5
作者：
Abdelwahed, H. G. [1 ,3 ]
El-Shewy, E. K. [2 ,3 ]
El-Rahman, A. A. [4 ]
Abdo, N. F. [2 ,5 ]
机构：
[1] Prince Sattam bin Abdulaziz Univ, Coll Sci & Humanities Al Kharj, Dept Phys, Al Kharj 11942, Saudi Arabia
[2] Taibah Univ, Al Madinah Al Munawarrah, Saudi Arabia
[3] Mansoura Univ, Fac Sci, Theoret Phys Grp, Mansoura, Egypt
[4] New Valley Univ, Fac Sci, Dept Phys, El Kharja 72714, Egypt
[5] Mansoura Univ, Fac Sci, Dept Math, Mansoura 35516, Egypt
来源：
ADVANCES IN SPACE RESEARCH | 2020年 / 65卷 / 01期
关键词：
Dust plasmas; Cylindrical Burgers; Dust cylindrical ion acoustic shocks; Nonthermal electrons; ACOUSTIC SOLITARY WAVES; TANH METHOD;
D O I：
10.1016/j.asr.2019.09.051
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
The propagating cylindrical shock dust ion wave (CDISW) in dusty four component plasma with three viscous component (ion and two polarity charged grains) has been introduced. The three dimensional (3D) Cylindrical Burgers (CB) equation is derived. The propagating cylindrical shock characteristics are established to becomes a very significantly improved by the supports of electron nonthermality, ion and negative (positive) kinematics viscosity coefficients. Furthermore, the shock strength depends on cylindrical directions. The obtained results may be profitable in understanding both the laboratory and space applications of plasmas. (C) 2019 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码：684 / 692
页数：9
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