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PARTICLE DIFFUSION ON VORTICES IN NEARLY INCOMPRESSIBLE MAGNETOHYDRODYNAMICS

机译:几乎不可压缩的磁氢动力学中的颗粒扩散

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摘要

Standard theory of energetic particle transport in magnetic irregularities treats the latter as weak random fluctuations described as linear MHD wave modes and does not include nonlinear coherent structures such as vortices. To address this shortcoming, a study of energetic particle diffusion in the heliosphere, taking into account scattering on vortices, is made. We consider vortices as nonlinear coherent planar two-dimensional structures orthogonal to the background magnetic field. They can be derived in the framework of nearly incompressible two-dimensional MHD for a subsonic plasma in the fluid frame with plasma beta β ≤ 1 and correspond to "zero-frequency" modes in the linear regime. Transport coefficients for energetic particles are evaluated using the Hamiltonian formalism and variational principles. Further applications for study of cosmic-ray transport in the heliosphere are discussed.
机译:磁不规则中高能粒子传输的标准理论将后者视为微弱的随机波动,描述为线性MHD波模式,并且不包括非线性相干结构(例如涡旋)。为了解决该缺点,进行了考虑到涡旋上的散射的高能粒子在日球中扩散的研究。我们将涡旋视为与背景磁场正交的非线性相干平面二维结构。它们可以在血浆ββ≤1的流体框架中的亚音速等离子体的几乎不可压缩的二维MHD框架中得出,并且对应于线性状态中的“零频率”模式。使用汉密尔顿形式主义和变分原理评估高能粒子的传输系数。讨论了在日光层中研究宇宙射线传输的更多应用。

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