Planetary Rotation Rate

Planetary Rotation Rate is a geophysical parameter that quantifies the angular velocity of a planet's spin about its axis, distinguishing it from orbital motion by characterizing the intrinsic rotational dynamics governing diurnal cycles, atmospheric circulation, and surface temperature distribution.

356

Publications

21.3K

Citations

1.4K

Authors

450

Institutions

Publications per year

2017–2026

72

Variants

Planetary Spin Rate

Authors

1.4K

  1. DV
    David Vokrouhlický

    Charles University, Czechia

    6 publications · 1.2K citations

    6

    h-index

  2. JM
    J. M. Aurnou

    University of California, Los Angeles, United States

    6 publications · 374 citations

    6

    h-index

  3. RK
    R. K. Ulrich

    University of California, Los Angeles, United States

    5 publications · 547 citations

    5

    h-index

  4. HM
    H. M. Antia

    Tata Institute of Fundamental Research, India

    5 publications · 342 citations

    5

    h-index

  5. MK
    M. K. Dougherty

    Imperial College London, United Kingdom

    5 publications · 305 citations

    5

    h-index

1–5 of 1.4K

Venues

  1. The Astrophysical Journal

    ApJ · 68 publications · 4.9K citations

    41

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 39 publications · 1.9K citations

    25

    h-index

  3. Geophysical Research Letters

    25 publications · 1K citations

    21

    h-index

  4. Icarus

    18 publications · 758 citations

    16

    h-index

  5. Astronomy and Astrophysics

    17 publications · 687 citations

    15

    h-index

1–5