Three-dimensional Atmospheric Models

Three-Dimensional Atmospheric Models is a computational modeling framework in stellar astrophysics that simulates the structure and dynamics of stellar atmospheres by solving radiative transfer and hydrodynamic equations across three spatial dimensions, thereby accounting for non-uniform temperature, velocity, and density structures arising from convection and other local phenomena unlike one- or two-dimensional approximations.

399

Publications

34.3K

Citations

1.2K

Authors

493

Institutions

Publications per year

2017–2026

80

Publications

399

1–5 of 399

Authors

1.2K

  1. MA
    M. Asplund

    Australian National University, Australia

    13 publications · 1.3K citations

    12

    h-index

  2. HL
    H.‐G. Ludwig

    Galaxies, Etoiles, Physique et Instrumentation, France

    12 publications · 586 citations

    12

    h-index

  3. RC
    R. Collet

    Aarhus University, Denmark

    9 publications · 950 citations

    9

    h-index

  4. AK
    A. Kučinskas

    Vilnius University, Lithuania

    8 publications · 218 citations

    8

    h-index

  5. BF
    B. Freytag

    Uppsala University, Sweden

    8 publications · 683 citations

    8

    h-index

1–5 of 1.2K

Venues

  1. The Astrophysical Journal

    ApJ · 47 publications · 6.2K citations

    36

    h-index

  2. Astronomy and Astrophysics

    43 publications · 3.5K citations

    31

    h-index

  3. Icarus

    14 publications · 556 citations

    14

    h-index

  4. Atmospheric chemistry and physics

    13 publications · 1.3K citations

    13

    h-index

  5. Journal of the Atmospheric Sciences

    15 publications · 1.1K citations

    13

    h-index

1–5