Galactic Magnetic Fields

Galactic Magnetic Fields is a large-scale magnetic phenomenon in the interstellar medium of galaxies, characterized by ordered and turbulent components that influence cosmic ray propagation, gas dynamics, and star formation processes through magnetohydrodynamic interactions.

2.8K

Publications

167.1K

Citations

7.1K

Authors

1.4K

Institutions

Publications per year

2017–2026

548

Authors

7.1K

  1. RB
    R. Beck

    Max Planck Institute for Radio Astronomy, Germany

    78 publications · 5.9K citations

    39

    h-index

  2. AS
    Anvar Shukurov

    Newcastle University, United Kingdom

    49 publications · 4K citations

    30

    h-index

  3. DD
    D. D. Sokoloff

    Lomonosov Moscow State University, Russia

    37 publications · 3.1K citations

    25

    h-index

  4. BM
    B. M. Gaensler

    The University of Sydney, Australia

    35 publications · 2.6K citations

    25

    h-index

  5. MH
    M. Haverkorn

    Radboud University Nijmegen, Netherlands

    40 publications · 2.4K citations

    25

    h-index

1–5 of 7.1K

Venues

  1. The Astrophysical Journal

    ApJ · 646 publications · 45.2K citations

    103

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    400 publications · 24.2K citations

    77

    h-index

  3. Astronomy and Astrophysics

    249 publications · 13.3K citations

    63

    h-index

  4. Nature

    59 publications · 6.7K citations

    37

    h-index

  5. Solar Physics

    70 publications · 3K citations

    32

    h-index

1–5