Solar Granulation Dynamics

Solar Granulation Dynamics is a physical phenomenon in solar physics characterized by the organized convective motion and temporal evolution of granular-scale plasma structures in the solar photosphere, driven by subsurface convection and marked by distinct upwelling centers and downdraft intergranular lanes.

143

Publications

8.2K

Citations

242

Authors

130

Institutions

Publications per year

2017–2026

12

Authors

242

  1. ÅN
    Åke Nordlund

    University of Copenhagen, Denmark

    8 publications · 1.6K citations

    8

    h-index

  2. JB
    José Bonet

    Universitat Politècnica de València, Spain

    8 publications · 381 citations

    8

    h-index

  3. AH
    A. Hanslmeier

    University of Graz, Austria

    8 publications · 349 citations

    8

    h-index

  4. JH
    J. Hirzberger

    Max Planck Institute for Solar System Research, Germany

    6 publications · 354 citations

    6

    h-index

  5. TR
    Th. Roudier

    Observatoire Midi-Pyrénées, France

    6 publications · 280 citations

    6

    h-index

1–5 of 242

Venues

  1. The Astrophysical Journal

    ApJ · 48 publications · 4.7K citations

    33

    h-index

  2. Astronomy and Astrophysics

    35 publications · 1.3K citations

    22

    h-index

  3. Solar Physics

    12 publications · 414 citations

    11

    h-index

  4. 6

    h-index

  5. The Astrophysical Journal Letters

    6 publications · 293 citations

    6

    h-index

1–5