Nonlinear density excitations in a magnetorotating relativistic plasma with warm ions and non-Maxwellian electrons

被引:8
作者
Ahmad, Ali [1 ]
Masood, W. [1 ,2 ]
机构
[1] Natl Ctr Phys, Shahdara Valley Rd, Islamabad, Pakistan
[2] COMSATS Inst Informat Technol, Pk Rd, Islamabad, Pakistan
关键词
ACOUSTIC SOLITARY WAVES; SOLAR-WIND; PROPAGATION; MAGNETOSPHERE; TEMPERATURE;
D O I
10.1063/1.4948421
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
Linear and nonlinear electrostatic ion acoustic waves in a weakly relativistic magnetorotating plasma in the presence of non-Maxwellian electrons and warm ions have been examined. The system under consideration has yielded two solutions, namely, the fast and slow acoustic modes which have been observed to depend on the streaming velocity, ion to electron temperature ratio, and the nonthermality parameter of the non-Maxwellian electrons. Using the multiple time scale analysis, we have derived the three dimensional nonlinear Zakharov-Kuznetsov equation and also presented its solution. Both compressive and rarefactive solitary structures have been found in consonance with the satellite observations. It has been observed that although the linear dispersion relation gives both fast and slow ion acoustic waves, the solitary structures form only for the fast acoustic mode. The dependence of the characteristics of the solitary structures on several plasma parameters has also been explored. The present investigation may be beneficial to understanding the rotating plasma environments such as those found in the planetary magnetospheres of Saturn and Jupiter. Published by AIP Publishing.
引用
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页数:7
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