Cosmic-ray Modulation

Cosmic-Ray Modulation is the phenomenon wherein the intensity and energy spectrum of galactic cosmic rays are systematically altered as they propagate through the heliosphere due to interactions with the solar wind, magnetic fields, and transient solar ejecta, resulting in an inverse correlation between cosmic-ray flux and solar activity levels.

790

Publications

39.3K

Citations

2.5K

Authors

542

Institutions

Publications per year

2017–2026

78

Variants

Galactic Cosmic-ray Modulation

Authors

2.5K

  1. MS
    M. S. Potgieter

    North-West University, South Africa

    89 publications · 4.5K citations

    42

    h-index

  2. WR
    W. R. Webber

    New Mexico State University, United States

    35 publications · 1.2K citations

    21

    h-index

  3. FB
    F. B. McDonald

    Goddard Space Flight Center, United States

    39 publications · 2K citations

    20

    h-index

  4. JR
    J. R. Jokipii

    University of Arizona, United States

    24 publications · 3.2K citations

    20

    h-index

  5. SE
    S. E. S. Ferreira

    North-West University, South Africa

    23 publications · 893 citations

    18

    h-index

1–5 of 2.5K

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 149 publications · 7.6K citations

    51

    h-index

  2. The Astrophysical Journal

    ApJ · 139 publications · 10.6K citations

    51

    h-index

  3. Advances in Space Research

    89 publications · 2.5K citations

    31

    h-index

  4. Solar Physics

    46 publications · 1.6K citations

    26

    h-index

  5. Geophysical Research Letters

    29 publications · 1.3K citations

    21

    h-index

1–5