Atmospheric sub-rotation

Last updated

Atmospheric sub-rotation or subrotation is the phenomenon where a planet's atmosphere rotates slower than the planet itself. It can be observed in the averaged motion of the Earth's troposphere and on the ice giant planets Neptune and Uranus. [1] [2] [3]

The reverse phenomenon is known as atmospheric super-rotation.

References

  1. Laraia, Anne L.; Schneider, Tapio (1 November 2015). "Superrotation in Terrestrial Atmospheres". Journal of the Atmospheric Sciences. 72 (11): 4281–4296. doi:10.1175/JAS-D-15-0030.1. ISSN   0022-4928.
  2. Duer-Milner, Keren; Gavriel, Nimrod; Galanti, Eli; Tziperman, Eli; Kaspi, Yohai (10 October 2025). "From gas to ice giants: A unified mechanism for equatorial jets". Science Advances. 11 (41): eads8899. doi:10.1126/sciadv.ads8899. ISSN   2375-2548. PMC   12513438 . PMID   41071886.{{cite journal}}: CS1 maint: article number as page number (link)
  3. Mendenhall, Brooks (6 November 2025). "Why do giant planet jet streams blow in opposite directions?". Astronomy Magazine. Retrieved 5 February 2026.

See also