Radiative Stability

Radiative Stability is a theoretical construct in atmospheric physics that denotes the condition under which a planetary atmosphere maintains a stable vertical temperature profile against radiative perturbations, distinguishing it from convective or dynamic stability mechanisms by focusing exclusively on radiative energy transfer and equilibrium adjustments.

100

Publications

10.3K

Citations

253

Authors

165

Institutions

Publications per year

2017–2026

28

Authors

253

  1. VB
    Viorel Bădescu

    Universitatea Națională de Știință și Tehnologie Politehnica București, Romania

    3 publications · 98 citations

    3

    h-index

  2. PH
    Peter H. Stone

    Brigham and Women's Hospital, United States

    3 publications · 412 citations

    3

    h-index

  3. IŞ
    Iuliana Şoriga

    University of Bucharest, Romania

    2 publications · 36 citations

    2

    h-index

  4. KE
    Kerry Emanuel

    Massachusetts Institute of Technology, United States

    2 publications · 221 citations

    2

    h-index

  5. MD
    Manuel Drees

    European Organization for Nuclear Research, Switzerland

    2 publications · 55 citations

    2

    h-index

1–5 of 253

Venues

  1. The Astrophysical Journal

    ApJ · 9 publications · 744 citations

    9

    h-index

  2. Journal of Cosmology and Astroparticle Physics

    JCAP · 5 publications · 235 citations

    5

    h-index

  3. 4

    h-index

  4. Journal of the Atmospheric Sciences

    4 publications · 522 citations

    4

    h-index

  5. Icarus

    3 publications · 93 citations

    3

    h-index

1–5