The DOI matches its Crossref record; 17 of the 17 references it cites were found in a registry or an index.
The Morphogenesis of Bands and Zonal Winds in the Atmospheres on the Giant Outer Planets
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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In the citing paper
“on one hand, the alternating jets on gas giant planets are 'shallow', existing above 10 bars or so [15-17]; on the other hand, zonal jets are 'deep', extending to tens of thousands of bars [18-22].”
From Deep rotating convection generates the polar hexagon on Saturn (2020) · cites this paper as [16]
In the citing paper
“This is likely driven by the topographical β effect, due to the spherical shell geometry, which is stronger near the equator, promoting strong axisymmetric jets, while, at higher latitudes, the β -effect decreases and the system approaches a rotating plane layer where the formation of giant vortices is favored”
From Deep rotating convection generates the polar hexagon on Saturn (2020) · cites this paper as [16]
Citations
Cites
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The emergence of jets and vortices in freely evolving, shallow-water turbulence on a sphere
Cho, J. Y., & Polvani, L. M. (1996) · Physics of Fluids · doi:10.1063/1.868929 · Cited by 235
Self-citationEnergy spectra and coherent structures in forced two-dimensional and beta-plane turbulence
Maltrud, M. E., & Vallis, G. K. (1991) · Journal of Fluid Mechanics · doi:10.1017/s0022112091002720 · Cited by 233
Atmospheric Dynamics of the Outer Planets
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Schou, J., Antia, H. M., Basu, S., Bogart, R. S., Bush, R. I., Chitre, S. M., Christensen-Dalsgaard, J., Mauro, M. P. D., Dziembowski, W. A., Eff‐Darwich, A., et al. (1998) · The Astrophysical Journal · doi:10.1086/306146 · Cited by 998
Atmospheric circulation and tides of “51 Pegasus b-like” planets
Showman, A. P., & Guillot, T. (2002) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20020101 · Cited by 617
Large-Scale Dynamics of the Convection Zone and Tachocline
Miesch, M. S. (2005) · Living Reviews in Solar Physics · doi:10.12942/lrsp-2005-1 · Cited by 348
Jovian atmospheric dynamics: an update after Galileo and Cassini
Vasavada, A. R., & Showman, A. P. (2005) · Reports on Progress in Physics · doi:10.1088/0034-4885/68/8/r06 · Cited by 329
Simulation of equatorial and high-latitude jets on Jupiter in a deep convection model
Heimpel, M., Aurnou, J., & Wicht, J. (2005) · Nature · doi:10.1038/nature04208 · Cited by 291
Metadata
- Authors
- Cho, J. Y.-K., & Polvani, L. M.
- Affiliations
- Columbia University (US)
- Venue
- Science
- Published
- 1996-07-19
- Volume
- 273
- Issue
- 5273
- Pages
- 335-337
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- 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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