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关于动力Alfven波的色散与朗道阻尼
引用本文:宋礼庭,卢先河.关于动力Alfven波的色散与朗道阻尼[J].地球物理学报,1999,42(2):145-153.
作者姓名:宋礼庭  卢先河
作者单位:1. 北京大学地球物理系 北京 100871; 2. 中国科学院空间科学和应用研究中心 北京 100080
基金项目:国家自然科学基金!49774249
摘    要:根据完全动力论理论,证明了可由简化漂移动力论方程求得动力Alfven波色散方程,即横向用磁流体力学方程,纵向用Vlasov方程,在初级近似下由此推导出适合于日冕和太阳风的色散关系和Landau阻尼,得到在性质上与MHD Alfven波完全不同的动力Alfven波,太阳风中Alfven湍流很容易由动力Alfven波演化而来。提出由动力Alfren波构筑太阳风高速流模型将更符合观测结果。

关 键 词:动力Alfven波  色散方程  Landau阻尼  Alfven湍流  
收稿时间:1998-09-30

ON THE DISPERSION AND LANDAU DAMPING OF THE KINETIC ALFVEN WAVE
SONG LI-TING.ON THE DISPERSION AND LANDAU DAMPING OF THE KINETIC ALFVEN WAVE[J].Chinese Journal of Geophysics,1999,42(2):145-153.
Authors:SONG LI-TING
Institution:1. Geophysical Department, Peking University, Beijing 100871, China; 2. Center for Space Science and Applied Research, CAS, Beijing 100080, China
Abstract:We prove that the dispersion equation of the kinetic Alfven wave obtained byfull kinetic theory can be derived from the so-called drift kinetic approximationequations. These are the hydrodynamic equations for motion transverse to the magneticfield and the Vlasov equation for longitudinal motion. On first approximation thedispersion relation and Landau damping derived by the dispersion equation for theconditions of the solar wind and corona. The kinetic Alfven wave in the nature isquite different from the MHD Alfven wave, so the Alfven turbulence in the solarwind can be easily formed by the kinetic Alfven waves. We present that constructingthe solar wind model from the kinetic Alfven waves will be more consistent with themeasurement.
Keywords:Kinetic Alfven wave  Dispersion equation  Landau damping  TheAlfven turbulence  
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