The DOI matches its Crossref record; 68 of the 72 references it cites were found in a registry or an index.
The deep wind structure of the giant planets: Results from an anelastic general circulation model
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In the citing paper
“The absence of momentum injection by eddies might be caused by injection of energy at smaller scales not resolvable by the measurements or might reinforce the idea that the jets are in fact deeply rooted structures driven by the internal convection [ Aurnou and Olson, 2001; Kaspi et al. 2009] making them insensitive at tropospheric level to the seasonal cycle”
From Dynamics of Saturn's polar regions (2015) · cites this paper as Kaspi et al. 2009
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 [22]
In the citing paper
“Their meridional eddy fluxes of angular momentum per unit volume (taking density variations into account) have a barotropic structure: they extend roughly along cylinders concentric with the planet's spin axis over the entire depth of the fluid, typically to pressures of order 10 6 bar (e.g., Kaspi et al. 2009, their Fig.10).”
From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Kaspi et al. 2009
In the citing paper
“Under these circumstances, convective plumes are columns aligned with M V surfaces because, as above, rapid rotation inhibits motion perpendicular to M V surfaces in the absence of viscous or other stresses (e.g., Busse 1976Busse , 1978;;Kaspi et al. 2009;Jones et al. 2009).”
From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Kaspi et al. 2009
In the citing paper
“If entropy deviations from an isentropic reference state are not small so that the anelastic approximation cannot be made, the thermal wind balance (13) becomes more complicated(Kaspi et al. 2009).”
From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Kaspi et al. 2009
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Jupiter’s atmospheric jet streams extend thousands of kilometres deep
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“…& Glatzmaier 2010; Schubert & Soderlund 2011), basic properties, such as the observed flow patterns in the atmosphere (Heimpel et al. 2005; Vasavada & Showman 2005; Kaspi et al. 2009; Gastine & Wicht 2012), still await explanations that are consistent with planetary structure and dynamo models.”
MethodResultFrom solar-like to antisolar differential rotation in cool stars
Gastine, T., Yadav, R. K., Morin, J., Reiners, A., & Wicht, J. (2013) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/slt162 · Cited by 204
Metadata
- Authors
- Kaspi, Y., Flierl, G. R., & Showman, A. P.
- Affiliations
- Massachusetts Institute of Technology (US)
- University of Arizona (US)
- Corresponding author
- Kaspi, Yohai
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 2009-08
- Volume
- 202
- Issue
- 2
- Pages
- 525-542
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W2087943296
- Cited by
- 149
- References
- 72
- Citations by year
- 2026: 5 · 2025: 5 · 2024: 9 · 2023: 7 · 2022: 6 · 2021: 8 · 2020: 15 · 2019: 13 · 2018: 9 · 2017: 16 · 2016: 6 · 2015: 11 · 2014: 10 · 2013: 9 · 2012: 8
- FWCI
- 3.36
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Icarus (publishedVersion)
- CaltechAUTHORS (California Institute of Technology) (submittedVersion)
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Engineering › Computational Mechanics › Fluid Dynamics and Turbulent Flows
- Keywords
- giant planet atmospheres, baroclinic vorticity, compressibility effects, vertical shear, thermal wind relation, equatorial superrotation, poleward heat transport, Rayleigh number, Jupiter, Saturn
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