Orbital-scale Climate Variability

Orbital-Scale Climate Variability is a paleoclimatological phenomenon characterized by long-term fluctuations in Earth's climate system driven by periodic changes in solar insolation resulting from variations in the planet's orbit, axial tilt, and precession, distinguishing it from shorter-term climate variability mechanisms.

150

Publications

22.4K

Citations

527

Authors

305

Institutions

Publications per year

2017–2026

44

Variants

Milankovitch-scale Climate Variability

Authors

527

  1. ZA
    Zhisheng An

    Institute of Earth Environment, China

    7 publications · 2.4K citations

    7

    h-index

  2. HC
    Hai Cheng

    University of Minnesota, United States

    7 publications · 2.2K citations

    7

    h-index

  3. RL
    R. Lawrence Edwards

    University of Minnesota, United States

    6 publications · 2.2K citations

    6

    h-index

  4. JI
    John Imbrie

    Harvard University, United States

    5 publications · 6.2K citations

    4

    h-index

  5. MF
    Marı́a Fernanda Sánchez Goñi

    École Pratique des Hautes Études, France

    4 publications · 423 citations

    4

    h-index

1–5 of 527

Venues

  1. Quaternary Science Reviews

    14 publications · 1.5K citations

    14

    h-index

  2. Earth and Planetary Science Letters

    10 publications · 1.1K citations

    10

    h-index

  3. Nature

    9 publications · 4.8K citations

    9

    h-index

  4. Geophysical Research Letters

    7 publications · 318 citations

    7

    h-index

  5. Global and Planetary Change

    6 publications · 262 citations

    6

    h-index

1–5