Numerical study of GCR proton transport
High Energy Astrophysical Phenomena
2024-11-08 v3
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.
Keywords
Cite
@article{arxiv.2211.08873,
title = {Numerical study of GCR proton transport},
author = {V. O Yurovsky and A. I. Peryatinskaya and I. Kudryashov},
journal= {arXiv preprint arXiv:2211.08873},
year = {2024}
}