Cited by 39Astro and Planetary ScienceIonosphere and magnetosphere dynamicsStellar, planetary, and galactic studies

The Saturnian ribbon feature—A baroclinically unstable model

Godfrey, D.A., Moore, V.·1986·Icarus

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Crossref · 10.1016/0019-1035(86)90026-6

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  • For jet centers at 35° and 30°, the jet equilibrates in a state more reminiscent of the Ribbon morphology than the Hexagon.

    “For the cases when the jet center is placed at 35 ° and 30 ° , the jet equilibrates in a state that is more reminiscent of the morphology of the Ribbon ( Godfrey & Moore 1986; Sayanagi et al. 2010 ) than that of the Hexagon.”

    From MEANDERING SHALLOW ATMOSPHERIC JET AS A MODEL OF SATURNʼS NORTH-POLAR HEXAGON (2015) · cites this paper as Godfrey & Moore 1986

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References 46 · Cited by 39

Authors
Godfrey, D. A., & Moore, V.
Affiliations
Imperial College London (GB)
Venue
Icarus
Publisher
Elsevier BV
Published
1986-11
Volume
68
Issue
2
Pages
313-343
ISSN
0019-1035 (ISSN-L)
OpenAlex
W2011540205
Cited by
39
References
46
Citations by year
2026: 1 · 2025: 1 · 2023: 1 · 2022: 1 · 2019: 3 · 2018: 2 · 2017: 1 · 2016: 1 · 2015: 3 · 2013: 1 · 2012: 1
FWCI
2.42
Type
journal article
Language
en
Open access
closed
Locations
Icarus (publishedVersion)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Ionosphere and magnetosphere dynamics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Keywords
Saturn, baroclinic instability, atmospheric waves, zonal circulation, meridional velocity, westerly jet, latitudinal thermal gradient

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