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Turbulent convection in rapidly rotating spherical shells: A model for equatorial and high latitude jets on Jupiter and Saturn
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“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 [26]
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“the number and the widths of the zonal jets are likely determined by the zonal flow strength and the topographic β effect [26].”
From Deep rotating convection generates the polar hexagon on Saturn (2020) · cites this paper as [26]
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“For example, deep-flow models that posit intrinsic heat fluxes as the sole driver of the flow can generate equatorial superrotation, but they use heat fluxes more than 10 6 times larger than those observed (e.g., Heimpel and Aurnou 2007).”
From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Heimpel and Aurnou 2007
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Metadata
- Authors
- Heimpel, M., & Aurnou, J.
- Affiliations
- University of Alberta (CA)
- University of California, Los Angeles (US)
- Corresponding author
- Heimpel, Moritz
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 2007-04
- Volume
- 187
- Issue
- 2
- Pages
- 540-557
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W2018072329
- Cited by
- 122
- References
- 58
- Citations by year
- 2026: 5 · 2025: 3 · 2024: 9 · 2023: 4 · 2022: 9 · 2021: 5 · 2020: 7 · 2019: 4 · 2018: 6 · 2017: 4 · 2016: 5 · 2015: 7 · 2014: 6 · 2013: 7 · 2012: 6
- FWCI
- 3.83
- Type
- journal article
- Language
- en
- Open access
- green
- escholarship.org
- Locations
- Icarus (publishedVersion)
- eScholarship (California Digital Library) (submittedVersion)
- 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 › Earth and Planetary Sciences › Geophysics › High-pressure geophysics and materials
- Keywords
- zonal jets, turbulent convection, Jupiter, Saturn, equatorial jet, geostrophic turbulence, tangent cylinder, beta parameter, jet width, planetary interiors
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
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