Theory of Cosmic Ray Transport in the Heliosphere

被引：0

作者：

N. Eugene Engelbrecht

F. Effenberger

V. Florinski

M. S. Potgieter

D. Ruffolo

R. Chhiber

A. V. Usmanov

J. S. Rankin

P. L. Els

机构：

[1] North-West University,Centre for Space Research

[2] National Institute for Theoretical and Computational Sciences (NITheCS),Institut für Theoretische Physik, IV

[3] Ruhr-Universität Bochum,Bay Area Environmental Research Institute

[4] NASA Research Park,Center for Space Plasma and Aeronomic Research (CSPAR) and Department of Space Science

[5] University of Alabama in Huntsville,Institute for Experimental and Applied Physics

[6] Christian-Albrechts University in Kiel,Department of Physics, Faculty of Science

[7] Mahidol University,Department of Physics and Astronomy, Bartol Research Institute

[8] University of Delaware,Department of Astrophysical Sciences

[9] NASA Goddard Space Flight Center,undefined

[10] Princeton University,undefined

来源：

Space Science Reviews | 2022年 / 218卷

关键词：

Cosmic rays; Diffusion; Turbulence;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

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

引用

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