Numerical study of GCR proton transport
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.
astro-ph.HE↗