Solar Magnetic Fields

Solar Magnetic Fields is a physical phenomenon consisting of magnetic fields generated by the motion of plasma within the Sun, characterized by their dynamic structure and influence on solar activity such as sunspots, flares, and coronal mass ejections.

10.1K

Publications

577.5K

Citations

10.7K

Authors

2K

Institutions

Publications per year

2017–2026

1.7K

Authors

10.7K

  1. SK
    S. K. Solanki

    Max Planck Institute for Solar System Research, Germany

    182 publications · 10.3K citations

    56

    h-index

  2. NR
    N. R. Sheeley

    United States Naval Research Laboratory, United States

    70 publications · 6.6K citations

    47

    h-index

  3. AM
    A. M. Title

    Lockheed Martin (United States), United States

    59 publications · 10.9K citations

    45

    h-index

  4. EN
    E. N. Parker

    University of Chicago, United States

    82 publications · 15.2K citations

    44

    h-index

  5. HW
    Haimin Wang

    New Jersey Institute of Technology, United States

    91 publications · 5.8K citations

    44

    h-index

1–5 of 10.7K

Venues

  1. The Astrophysical Journal

    ApJ · 2.9K publications · 197.5K citations

    182

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 1.1K publications · 83.2K citations

    132

    h-index

  3. Astronomy and Astrophysics

    906 publications · 42.2K citations

    93

    h-index

  4. Solar Physics

    662 publications · 41.9K citations

    87

    h-index

  5. The Astrophysical Journal Letters

    361 publications · 18.1K citations

    71

    h-index

1–5