http://arxiv.org/abs/2211.08873
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.
Y. V.O., P. I. and K. I.A
Thu, 17 Nov 22
9/63
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