Sunspot Magnetic Fields

Sunspot Magnetic Fields is a solar magnetic field configuration characterized by intense, localized magnetic flux concentrations that inhibit convective energy transport, forming in active regions of the Sun and manifesting as dark, cooler areas on the photosphere known as sunspots.

512

Publications

34K

Citations

697

Authors

264

Institutions

Publications per year

2017–2026

44

Authors

697

  1. SK
    S. K. Solanki

    Max Planck Institute for Solar System Research, Germany

    30 publications · 1.3K citations

    22

    h-index

  2. BW
    B. W. Lites

    NSF NCAR High Altitude Observatory, United States

    18 publications · 1.8K citations

    17

    h-index

  3. AL
    A. Lagg

    Max Planck Institute for Solar System Research, Germany

    16 publications · 759 citations

    15

    h-index

  4. RS
    R. Schlichenmaier

    Institut für Sonnenphysik, Germany

    15 publications · 633 citations

    15

    h-index

  5. MC
    M. Collados

    Instituto de Astrofísica de Canarias, Spain

    15 publications · 1K citations

    15

    h-index

1–5 of 697

Venues

  1. The Astrophysical Journal

    ApJ · 154 publications · 12.8K citations

    62

    h-index

  2. Solar Physics

    77 publications · 6.3K citations

    37

    h-index

  3. Astronomy and Astrophysics

    73 publications · 3.3K citations

    35

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    23 publications · 1.6K citations

    16

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 9 publications · 268 citations

    9

    h-index

1–5