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Pitch-angle scattering in magnetostatic turbulence. I. Test-particle simulations and the validity of analytical results

机译:静磁湍流中的俯仰角散射。 I.测试粒子   模拟和分析结果的有效性

摘要

Context. Spacecraft observations have motivated the need for a refineddescription of the phase-space distribution function. Of particular importanceis the pitch-angle diffusion coefficient that occurs in the Fokker-Plancktransport equation. Aims. Simulations and analytical test-particle theories arecompared to verify the diffusion description of particle transport, which doesnot allow for non-Markovian behavior. Methods. A Monte-Carlo simulation codewas used to trace the trajectories of test particles moving in turbulentmagnetic fields. From the ensemble average, the pitch-angle Fokker-Planckcoefficient is obtained via the mean square displacement. Results. It is shownthat, while excellent agreement with analytical theories can be obtained forslab turbulence, considerable deviations are found for isotropic turbulence. Inaddition, all Fokker-Planck coefficients tend to zero for high time values.
机译:上下文。航天器的观测激发了对相空间分布函数的精确描述的需求。特别重要的是在Fokker-Plancktransport方程中出现的俯仰角扩散系数。目的仿真和分析测试粒子理论进行了比较,以验证粒子传输的扩散描述,这不允许非马尔可夫行为。方法。使用蒙特卡罗模拟代码来跟踪在湍流磁场中移动的测试粒子的轨迹。从集合平均,通过均方位移获得俯仰角福克-普朗克系数。结果。结果表明,虽然对于平板湍流可以获得与分析理论的极好的一致性,但是对于各向同性湍流却发现了相当大的偏差。另外,对于高时间值,所有福克-普朗克系数都趋于零。

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