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Akarsh Goyal,Ishan Khandelwal,Rahul Anand,Anan Srivastava,P. Swarnalathais occurs is unclear. Despite the apparent success of the theory, there is no single choice for the parameters which describe cosmic ray behavior, which can account for all of the observed temporal and spatial variations, spectra, and electron vs. ion behavior.

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Anisotropic Subgrid-Scale Modelling: Comparison of LES with High Resolution DNS and Statistical Thethe approach, and to prepare improved anisotropic subgrid-scale modelling, we compare the results of high Reynolds number large eddy simulations based on this model to energy density spectra obtained at lower Reynolds number by direct numerical simulations, and to spectra obtained by a recent two-po

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