Cosmic-ray Diffusion

Cosmic-Ray Diffusion is a theoretical framework in astrophysics that describes the stochastic propagation of high-energy cosmic-ray particles through turbulent interstellar magnetic fields, distinguished from other transport mechanisms by its reliance on spatial and momentum-space diffusion coefficients derived from particle-scattering processes.

915

Publications

57.7K

Citations

1.5K

Authors

597

Institutions

Publications per year

2017–2026

169

Authors

1.5K

  1. JR
    J. R. Jokipii

    University of Arizona, United States

    41 publications · 6.1K citations

    28

    h-index

  2. MS
    M. S. Potgieter

    North-West University, South Africa

    32 publications · 1.6K citations

    24

    h-index

  3. DM
    D. Maurin

    Centre National de la Recherche Scientifique, France

    24 publications · 1.6K citations

    22

    h-index

  4. AS
    A. Shalchi

    Ruhr University Bochum, Germany

    34 publications · 1.6K citations

    22

    h-index

  5. RS
    R. Schlickeiser

    Ruhr University Bochum, Germany

    23 publications · 801 citations

    18

    h-index

1–5 of 1.5K

Venues

  1. The Astrophysical Journal

    ApJ · 221 publications · 20K citations

    67

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    70 publications · 4.6K citations

    43

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 81 publications · 4.2K citations

    38

    h-index

  4. Astronomy and Astrophysics

    59 publications · 3.5K citations

    36

    h-index

  5. Advances in Space Research

    42 publications · 1.4K citations

    22

    h-index

1–5