Solar Supergranulation

Solar Supergranulation is a large-scale convective flow pattern in the solar photosphere characterized by horizontal plasma motions organized into cellular structures approximately 30,000 kilometers in diameter, distinguishing it from smaller-scale granulation and mesogranulation features through its size, lifetime, and role in advecting magnetic fields across the Sun’s surface.

267

Publications

14.9K

Citations

409

Authors

214

Institutions

Publications per year

2017–2026

27

Authors

409

  1. LR
    L. R. Bellot Rubio

    Instituto de Astrofísica de Andalucía, Spain

    13 publications · 695 citations

    13

    h-index

  2. TR
    Th. Roudier

    Observatoire Midi-Pyrénées, France

    12 publications · 339 citations

    11

    h-index

  3. LG
    L. Gizon

    Max Planck Institute for Solar System Research, Germany

    11 publications · 617 citations

    10

    h-index

  4. AM
    A. M. Title

    Lockheed Martin (United States), United States

    10 publications · 785 citations

    10

    h-index

  5. MR
    M. Rieutord

    Centre National de la Recherche Scientifique, France

    11 publications · 439 citations

    10

    h-index

1–5 of 409

Venues

  1. The Astrophysical Journal

    ApJ · 111 publications · 8.9K citations

    48

    h-index

  2. Astronomy and Astrophysics

    43 publications · 1.4K citations

    25

    h-index

  3. Solar Physics

    22 publications · 670 citations

    17

    h-index

  4. The Astrophysical Journal Letters

    12 publications · 480 citations

    11

    h-index

  5. 10

    h-index

1–5