...
首页> 外文期刊>Physics of plasmas >Dust-acoustic waves and stability in the permeating dusty plasma. II. Power-law distributions
【24h】

Dust-acoustic waves and stability in the permeating dusty plasma. II. Power-law distributions

机译:尘埃声波和渗透尘埃等离子体的稳定性。二。幂律分布

获取原文
获取原文并翻译 | 示例

摘要

The dust-acoustic waves and the stability theory for the permeating dusty plasma with power-law distributions are studied by using nonextensive q-statistics. In two limiting physical cases, when the thermal velocity of the flowing dusty plasma is much larger than, and much smaller than the phase velocity of the waves, we derived the dust-acoustic wave frequency, the instability growth rate, and the instability critical flowing velocity. As compared with the formulae obtained in part I [Gong, Phys. Plasmas 19, 043704 (2012)], all formulae of the present cases and the resulting plasma characteristics are q-dependent, and the power-law distribution of each plasma component of the permeating dusty plasma has a different q-parameter and thus has a different nonextensive effect. Further, we make numerical analyses of an example that a cometary plasma tail is passing through the interplanetary space dusty plasma and we show that these power-law distributions have significant effects on the plasma characteristics of this kind of plasma environment.
机译:利用非扩展q统计量,研究了具有幂律分布的粉尘等离子体的粉尘声波和稳定性理论。在两种有限的物理情况下,当流动的尘埃等离子体的热速度远大于波的相速度,并且远小于波的相速度时,我们可以推导出尘埃声波的频率,不稳定的增长率和不稳定的临界流动速度。与在第一部分中获得的公式相比[Gong,Phys。 Plasmas 19,043704(2012)],本案例的所有公式及其产生的等离子体特性均与q有关,并且渗透尘埃等离子体的各个等离子体成分的幂律分布具有不同的q参数,因此具有不同的不广泛作用。此外,我们对一个示例进行了数值分析,该示例表明彗星等离子体尾部正穿过行星际空间尘埃等离子体,并且我们证明了这些幂律分布对这种等离子体环境的等离子体特性具有重要影响。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号