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G. Zimbardo S. Perri P. Pommois P. Veltri 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
The transport of energetic particles in the presence of magnetic turbulence can exhibit a variety of regimes different from the standard quasilinear diffusion. Here we discuss a number of solar and space problems where nonquasilinear diffusion is found, and then we illustrate anomalous transport regimes, for which the mean square deviation grows nonlinearly with time. In particular, we concentrate on superdiffusive regimes, and show what is the theoretical framework which is to be used to describe superdiffusion. We discuss the results of numerical simulations which show that superdiffusive and subdiffusive regimes are possible, and describe data analyses which allow to single out the superdiffusive transport from the observation of energetic particle profiles upstream of interplanetary shocks. The implications of superdiffusion on the efficiency of wave particle interactions are also discussed. 相似文献
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Cross field diffusion of energetic particles (cosmic rays) in a two-dimensional static magnetic field turbulence is studied
performing test particle simulations. Qualitatively different diffusion processes are observed depending on the ratio of Larmor
radius (ρ) to the correlation length (λ) of the magnetic field fluctuations. The diffusion is found to be composed of several
regimes with distinct statistical properties, which can be characterized using Levy statistics.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
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对具有高阶传递函数的某控制系统仪器 ,采用延长序列的傅立叶变换方法 ,准确、快速地得到了其动态频率特性 ,并用改进的Levy方法准确辨识出了系统模型。 相似文献
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