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Non-Gaussian probability distribution functions in two-dimensional magnetohydrodynamic turbulence

机译:二维磁流体动力湍流中的非高斯概率分布函数

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摘要

Intermittency in MHD turbulence has been analyzed using high-resolution 2D numerical simulations. We show that the Probability Distribution Functions (PDFs) of the fluctuations of the Elsasser fields, magnetic field and velocity field depend on the scale at hand, that is they are self-affine. The departure of the PDFs from a Gaussian function can be described through the scaling behavior of a single parameter lambda(r)(2) obtained by fitting the PDFs with a given curve stemming from the analysis of a multiplicative model by Castaing et al. (Physica D, 46 (1990) 177). The scaling behavior of the parameter lambda(r)(2) can be used to extract information about the intermittency. A comparison of intermittency properties in different MHD turbulent flows is also performed. [References: 21]
机译:已使用高分辨率2D数值模拟分析了MHD湍流的间歇性。我们表明,Elsasser场,磁场和速度场的涨落的概率分布函数(PDFs)取决于当前的尺度,即它们是自仿射的。 PDF与高斯函数的偏离可以通过单参数lambda(r)(2)的缩放行为来描述,该参数是通过用Castaing等人对乘法模型的分析得出的给定曲线拟合PDF来获得的。 (Physica D,46(1990)177)。参数lambda(r)(2)的缩放比例行为可用于提取有关间歇性的信息。还对不同MHD湍流中的间歇性进行了比较。 [参考:21]

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