Cited by 124Astro and Planetary ScienceFluid Dynamics and Turbulent FlowsIonosphere and magnetosphere dynamics

Interaction between eddies and mean flow in Jupiter’s atmosphere: Analysis of Cassini imaging data.

Salyk, Colette, Ingersoll, Andrew P., Lorre, Jean, Vasavada, Ashwin, Del Genio, Anthony D.·2006·Icarus

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Crossref · 10.1016/j.icarus.2006.08.007

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19 of 19 references verified0 citation errors · 0 not checkable

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  • Eddy angular momentum fluxes inferred from tracking cloud features in Jupiter's and Saturn's upper tropospheres indicate that the mean conversion rate from eddy to mean-flow kinetic energy is of order 10^-5 W m^-3.

    “But the eddy angular momentum fluxes inferred from tracking cloud features in Jupiter's and Saturn's upper tropospheres indicate that the mean conversion rate from eddy to mean-flow kinetic energy is of order 10 25 W m 23 (Ingersoll et al. 1981;Salyk et al. 2006;Del Genio et al. 2007).”

    From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Salyk et al. 2006

  • Such angular momentum transport from retrograde into prograde jets has indeed been observed on Jupiter and Saturn.

    “Such angular momentum transport from retrograde into prograde jets has indeed been observed on Jupiter and Saturn (Ingersoll et al. 1981;Salyk et al. 2006;Del Genio et al. 2007).”

    From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Salyk et al. 2006

  • This angular momentum transport has a baroclinic structure and, in the Jupiter and Saturn simulations, is in structure and magnitude consistent with observations.

    “It has a baroclinic structure and, in the Jupiter and Saturn simulations, is in structure and magnitude consistent with observations (cf.Ingersoll et al. 1981;Salyk et al. 2006;Del Genio et al. 2007).”

    From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Salyk et al. 2006

  • The same pattern of eddy angular momentum fluxes and mean meridional mass flux is almost certainly true on Jupiter and Saturn, where similar eddy angular momentum fluxes in the upper troposphere have been observed.

    “The same is almost certainly true on Jupiter and Saturn, where similar eddy angular momentum fluxes in the upper troposphere have been observed (Salyk et al. 2006;Del Genio et al. 2007).”

    From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Salyk et al. 2006

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Authors
Salyk, C., Ingersoll, A. P., Lorre, J., Vasavada, A., & Del Genio, A. D.
Affiliations
  • California Institute of Technology (US)
  • Jet Propulsion Laboratory (US)
Corresponding author
Salyk, Colette
Venue
Icarus
Publisher
Elsevier BV
Published
2006-12
Volume
185
Issue
2
Pages
430-442
ISSN
0019-1035 (ISSN-L)
OpenAlex
W2087339719
Cited by
124
References
20
Citations by year
2026: 4 · 2025: 6 · 2024: 7 · 2023: 4 · 2022: 6 · 2021: 7 · 2020: 17 · 2019: 3 · 2018: 10 · 2017: 4 · 2016: 1 · 2015: 5 · 2014: 4 · 2013: 9 · 2012: 5
FWCI
4.22
Type
journal article
Language
en
Open access
closed
Locations
  • Icarus (publishedVersion)
  • CaltechAUTHORS (California Institute of Technology) (submittedVersion)
Funders
National Aeronautics and Space Administration
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
  • Physical Sciences › Engineering › Computational Mechanics › Fluid Dynamics and Turbulent Flows
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Ionosphere and magnetosphere dynamics
Keywords
Jupiter, eddy-mean flow interaction, eddy momentum flux, zonal wind, zonal flows, Cassini flybys, Great Red Spot, atmospheric dynamics

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