Orbital Forcing Simulations

Orbital Forcing Simulations is a paleoclimate modeling method that systematically computes the climatic effects of Earth's orbital variations—such as eccentricity, axial tilt, and precession—by isolating their influence on the distribution and intensity of incoming solar radiation over geologic time scales.

154

Publications

15.3K

Citations

604

Authors

306

Institutions

Publications per year

2017–2026

33

Authors

604

  1. PB
    Pascale Braconnot

    Laboratoire des Sciences du Climat et de l'Environnement, France

    9 publications · 1.2K citations

    9

    h-index

  2. BL
    Bette L. Otto‐Bliesner

    NSF National Center for Atmospheric Research, United States

    8 publications · 1.6K citations

    8

    h-index

  3. GL
    Gerrit Lohmann

    Alfred-Wegener-Institut Helmholtz-Zentrum für Polar- und Meeresforschung, Germany

    7 publications · 605 citations

    7

    h-index

  4. JE
    John E. Kutzbach

    University of Wisconsin–Madison, United States

    7 publications · 1.4K citations

    7

    h-index

  5. SP
    Sandy P. Harrison

    University of Reading, United Kingdom

    7 publications · 704 citations

    7

    h-index

1–5 of 604

Venues

  1. Climate of the past

    17 publications · 927 citations

    16

    h-index

  2. Quaternary Science Reviews

    11 publications · 1.2K citations

    11

    h-index

  3. Palaeogeography Palaeoclimatology Palaeoecology

    11 publications · 525 citations

    11

    h-index

  4. Nature

    11 publications · 2.5K citations

    11

    h-index

  5. Journal of Climate

    9 publications · 521 citations

    9

    h-index

1–5