Galactic Cosmic Rays

Galactic Cosmic Rays is a class of high-energy charged particles, predominantly protons and atomic nuclei, of extrasolar origin that originate from outside the solar system and propagate through the Milky Way galaxy, distinguished from solar and anomalous cosmic rays by their higher energies and nucleosynthetic signatures indicative of supernova and other galactic astrophysical processes.

3.1K

Publications

184.9K

Citations

11.9K

Authors

1.7K

Institutions

Publications per year

2017–2026

595

Authors

11.9K

  1. MS
    M. S. Potgieter

    North-West University, South Africa

    46 publications · 2.8K citations

    30

    h-index

  2. IU
    Ilya Usoskin

    University of Oulu, Finland

    40 publications · 3.5K citations

    29

    h-index

  3. JR
    J. R. Jokipii

    University of Arizona, United States

    38 publications · 3.9K citations

    27

    h-index

  4. JH
    J.R. Hörandel

    Radboud University Nijmegen, Netherlands

    33 publications · 4.6K citations

    27

    h-index

  5. PB
    Pasquale Blasi

    Arcetri Astrophysical Observatory, Italy

    33 publications · 3.9K citations

    27

    h-index

1–5 of 11.9K

Venues

  1. The Astrophysical Journal

    ApJ · 618 publications · 44.7K citations

    107

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 216 publications · 12.4K citations

    62

    h-index

  3. Astronomy and Astrophysics

    118 publications · 6.9K citations

    52

    h-index

  4. 45

    h-index

  5. Physical Review Letters

    PRL · 71 publications · 6.4K citations

    42

    h-index

1–5