Propagation of radiation in fluctuating multiscale plasmas. I. Kinetic theory

被引：0

作者：

Tyshetskiy, Yu. ^{[1
]}

Singh, Kunwar Pal ^{[1
]}

Thirunavukarasu, A. ^{[1
]}

Robinson, P. A. ^{[1
]}

Cairns, Iver H. ^{[1
]}

机构：

[1] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia

来源：

PHYSICS OF PLASMAS | 2012年 / 19卷 / 11期

基金：

澳大利亚研究理事会;

关键词：

CLUMPY LANGMUIR-WAVES; III RADIO-SOURCES; HARMONIC EMISSION; MODE CONVERSION; BURSTS; BEAM; PARAMETERS; FREQUENCY; GROWTH;

D O I：

10.1063/1.4767640

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：

A theory for propagation of radiation in a large scale plasma with small scale fluctuations is developed using a kinetic description in terms of the probability distribution function of the radiation in space, time, and wavevector space. Large scale effects associated with spatial variations in the plasma density and refractive index of the plasma wave modes and small scale effects such as scattering of radiation by density clumps in fluctuating plasma, spontaneous emission, damping, and mode conversion are included in a multiscale kinetic description of the radiation. Expressions for the Stokes parameters in terms of the probability distribution function of the radiation are used to enable radiation properties such as intensity and polarization to be calculated. (C) 2012 American Institute of Physics. [http://dx.doi.org/10.1063/1.4767640]

引用

页数：18

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