Theory of Cosmic Ray Transport in the Heliosphere

• DOI: 10.1007/s11214-022-00896-1
• Publication Date: 2022-05-25T10:03:13Z
• Authors: N. Eugene Engelbr...; F. Effenberger; V. Florinski; M. S. Potgieter; D. Ruffolo; R. Chhiber; A. V. Usmanov; J. S. Rankin; P. L. Els
• Keywords: Heliosphere

Abstract Modelling the transport of cosmic rays (CRs) in heliosphere represents a global challenge field heliophysics, that such study, if it were to be performed from first principles, requires careful modelling both large scale heliospheric plasma quantities (such as structure heliosphere, or magnetic field) and small various turbulence-related quantities). Here, recent advances our understanding galactic are reviewed, with an emphasis on new developments pertaining their coefficients, special novel theoretical numerical simulation results, well CR studies employ them. Furthermore, brief reviews given progress focused modelling, non-diffusive transport.