Spectra of high-frequency waves in hot magnetized plasmas

被引:3
|
作者
Ledenev V.G. [1 ,2 ]
Tirsky V.V. [1 ,2 ]
机构
[1] Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences, Irkutsk
[2] Irkutsk Branch, Institute of Laser Physics, Russian Academy of Sciences, Irkutsk
基金
俄罗斯基础研究基金会;
关键词
Dispersion Curve; Dispersion Equation; Dispersion Characteristic; Cold Plasma; Anomalous Dispersion;
D O I
10.1007/s11141-006-0056-7
中图分类号
学科分类号
摘要
On the basis of numerical solution of the dispersion equation, we obtain the spectra of weakly damped high-frequency waves in a hot magnetized plasma for the case where the electron cyclotron frequency ωHe is below the plasma frequency ωpe. It is shown that the longitudinal wave propagating at an angle to the magnetic field evolves into the slow extraordinary wave for the refractive index n ≤ 1. For n ≫ 1, the longitudinal-wave frequency increases with the refractive index, and the wave evolves into the wave with anomalous dispersion if the angle θ between the wave vector and the magnetic field is close to 90°. In the same range of θ angles, Bernstein modes appear in the spectrum of plasma eigenmode oscillations. © Springer Science+Business Media, Inc. 2006.
引用
收藏
页码:231 / 238
页数:7
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