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arXiv · 2211.08873

Numerical study of GCR proton transport

V. O Yurovsky·A. I. Peryatinskaya·I. Kudryashov
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Abstract

The paper numerically investigates the propagation of galactic cosmic rays in a model magnetic field, which is a composition of an isotropic turbulent field with the Kolmogorov turbulence spectrum and a regular constant field. The dependence of the diffusion tensor components on the particle energy is studied. It is shown that the transport anisotropy increases with decreasing energy.

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V. O Yurovsky, A. I. Peryatinskaya, I. Kudryashov. 2022-11-16. Numerical study of GCR proton transport. https://arxiv.org/abs/2211.08873

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