Solar Dynamo Processes

Solar Dynamo Processes is a theoretical framework in astrophysics that explains the generation and modulation of the Sun's large-scale magnetic field through the interaction of convective plasma motions and differential rotation within the solar interior.

840

Publications

58.5K

Citations

1.3K

Authors

524

Institutions

Publications per year

2017–2026

155

Authors

1.3K

  1. RH
    R. H. Cameron

    Max Planck Institute for Solar System Research, Germany

    27 publications · 1.8K citations

    24

    h-index

  2. AR
    Arnab Rai Choudhuri

    Indian Institute of Science Bangalore, India

    24 publications · 2.2K citations

    21

    h-index

  3. DD
    D. D. Sokoloff

    Lomonosov Moscow State University, Russia

    24 publications · 1K citations

    19

    h-index

  4. PA
    Peter A. Gilman

    NSF NCAR High Altitude Observatory, United States

    24 publications · 2.1K citations

    19

    h-index

  5. AB
    Axel Brandenburg

    Stockholm University, Sweden

    20 publications · 1.5K citations

    19

    h-index

1–5 of 1.3K

Venues

  1. The Astrophysical Journal

    ApJ · 213 publications · 20.2K citations

    75

    h-index

  2. Astronomy and Astrophysics

    103 publications · 6.5K citations

    44

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    55 publications · 2.6K citations

    29

    h-index

  4. Solar Physics

    41 publications · 4.1K citations

    27

    h-index

  5. The Astrophysical Journal Letters

    26 publications · 1.5K citations

    23

    h-index

1–5