Cited by 131Astro and Planetary ScienceFluid Dynamics and Turbulent FlowsStellar, planetary, and galactic studies

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The Morphogenesis of Bands and Zonal Winds in the Atmospheres on the Giant Outer Planets

Cho, James Y-K., Polvani, Lorenzo M.·1996·Science

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Abstract

The atmospheres of Jupiter, Saturn, Uranus, and Neptune were modeled as shallow layers of turbulent fluid overlying a smooth, spherical interior. With only the observed values of radius, rotation rate, average wind velocity, and mean layer thickness as model parameters, bands and jets spontaneously emerged from random initial conditions. The number, width, and amplitude of the jets, as well as the dominance of anticyclonic vortices, are in good agreement with observations for all four planets.

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Authors: Cho, J. Y.-K., & Polvani, L. M.
Affiliations: Columbia University (US)
ORCID: Cho, James Y-K.
Polvani, Lorenzo M.
Venue: Science
Publisher: American Association for the Advancement of Science (AAAS)
Published: 1996-07-19
Volume: 273
Issue: 5273
Pages: 335-337
ISSN: 0036-8075 (ISSN-L)
1095-9203
DOI: 10.1126/science.273.5273.335
OpenAlex: W2014901376
Cited by: 131
References: 17
Citations by year: 2026: 3 · 2025: 5 · 2024: 4 · 2023: 1 · 2022: 4 · 2021: 3 · 2020: 10 · 2018: 2 · 2017: 4 · 2016: 2 · 2015: 3 · 2014: 6 · 2013: 8 · 2012: 4
FWCI: 5.03
Type: journal article
Language: en
Open access: closed
Locations: Science (publishedVersion)
PubMed (publishedVersion)
Topics: Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
Physical Sciences › Engineering › Computational Mechanics › Fluid Dynamics and Turbulent Flows
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Keywords: giant planet atmospheres, zonal jets, jet stream, atmospheric bands, morphogenesis, spontaneous pattern formation, anticyclonic vortices, Jupiter, Saturn, Uranus, Neptune

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The Morphogenesis of Bands and Zonal Winds in the Atmospheres on the Giant Outer Planets

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