Orbital Parameter Variations

Orbital Parameter Variations is a theoretical construct in climatology that specifies the gradual changes in Earth's orbital characteristics—namely eccentricity, axial tilt (obliquity), and precession—distinguishing it from other climate forcings by describing the periodic modulations in solar insolation caused by celestial mechanics underlying Milankovitch cycles.

317

Publications

31.6K

Citations

1.1K

Authors

521

Institutions

Publications per year

2017–2026

67

Authors

1.1K

  1. ML
    Marie‐France Loutre

    UCLouvain, Belgium

    5 publications · 759 citations

    5

    h-index

  2. WF
    William F Ruddiman

    University of Virginia, United States

    4 publications · 1.1K citations

    4

    h-index

  3. SM
    S. M. Ruciński

    University of Toronto, Canada

    4 publications · 171 citations

    4

    h-index

  4. JL
    J. Laskar

    Institut de Mécanique Céleste et de Calcul des Éphémérides, France

    4 publications · 1.1K citations

    4

    h-index

  5. BW
    B. W. Stappers

    University of Manchester, United Kingdom

    4 publications · 62 citations

    4

    h-index

1–5 of 1.1K

Venues

  1. Astronomy and Astrophysics

    21 publications · 840 citations

    18

    h-index

  2. The Astrophysical Journal

    ApJ · 23 publications · 1.2K citations

    18

    h-index

  3. 16

    h-index

  4. The Astronomical Journal

    AJ · 19 publications · 725 citations

    15

    h-index

  5. Geophysical Research Letters

    13 publications · 393 citations

    12

    h-index

1–5