In the report numerical investigation of the propagation of galactic cosmic rays in a model magnetic field is discussed. The magnetic field is modeled as 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.
Volume 444 -
38th International Cosmic Ray Conference (ICRC2023) -
Cosmic-Ray Physics (Indirect, CRI)
Numerical study of GCR proton transport
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Pre-published on:
July 25, 2023
Published on:
September 27, 2024
Abstract
DOI: https://doi.org/10.22323/1.444.0201
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.