Stellar Granulation

Stellar Granulation is a convective surface phenomenon in stellar atmospheres characterized by a pattern of bright, cell-like structures surrounded by darker lanes, resulting from the upward transport of heat via hot plasma rising in the centers of granules and cooler plasma sinking at their boundaries.

92

Publications

4.8K

Citations

332

Authors

155

Institutions

Publications per year

2017–2026

14

Authors

332

  1. DF
    David F. Gray

    Western University, Canada

    8 publications · 398 citations

    8

    h-index

  2. HL
    H.‐G. Ludwig

    Galaxies, Etoiles, Physique et Instrumentation, France

    7 publications · 227 citations

    7

    h-index

  3. TK
    T. Kallinger

    University of Vienna, Austria

    6 publications · 658 citations

    6

    h-index

  4. ÅN
    Åke Nordlund

    University of Copenhagen, Denmark

    6 publications · 197 citations

    6

    h-index

  5. RA
    R. A. García

    Commissariat à l'Énergie Atomique et aux Énergies Alternatives, France

    6 publications · 1K citations

    6

    h-index

1–5 of 332

Venues

  1. Astronomy and Astrophysics

    24 publications · 1.4K citations

    20

    h-index

  2. The Astrophysical Journal

    ApJ · 18 publications · 1.2K citations

    16

    h-index

  3. Solar Physics

    8 publications · 196 citations

    8

    h-index

  4. 4

    h-index

  5. The Astrophysical Journal Letters

    4 publications · 193 citations

    4

    h-index

1–5