Cited by 19Astro and Planetary ScienceFluid Dynamics and Turbulent FlowsIonosphere and magnetosphere dynamics

Saturn’s Northern Hemisphere Ribbon: Simulations and Comparison with the Meandering Gulf Stream

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Sayanagi, Kunio M., Morales-Juberías, Raúl, Ingersoll, Andrew P.·2010·Journal of the Atmospheric Sciences

Abstract

Voyager observations of Saturn in 1980–81 discovered a wavy feature engirdling the planet at 47°N planetographic latitude. Its latitude coincides with that of an eastward jet stream, which is the second fastest on Saturn after the equatorial jet. The 47°N jet’s wavy morphology is unique among the known atmospheric jets on the gas giant planets. Since the Voyagers, it has been seen in every high-resolution image of this latitude for over 25 years and has been termed the Ribbon. The Ribbon has been interpreted as a dynamic instability in the jet stream. This study tests this interpretation and uses forward modeling to explore the observed zonal wind profile’s stability properties. Unforced, initial-value numerical experiments are performed to examine the nonlinear evolution of the jet stream. Parameter variations show that an instability occurs when the 47°N jet causes reversals in the potential vorticity (PV) gradient, which constitutes a violation of the Charney–Stern stability criterion. After the initial instability development, the simulations demonstrate that the instability’s amplitude nonlinearly saturates to a constant when the eddy generation by the instability is balanced by the destruction of the eddies. When the instability saturates, the zonal wind profile approaches neutral stability according to Arnol’d’s second criterion, and the jet’s path meanders in a Ribbon-like manner. It is demonstrated that the meandering of the 47°N jet occurs over a range of tropospheric static stability and background wind speed. The results here show that a nonlinearly saturated shear instability in the 47°N jet is a viable mechanism to produce the Ribbon morphology. Observations do not yet have the temporal coverage to confirm the creation and destruction of eddies, but these simulations predict that this is actively occurring in the Ribbon region. Similarities exist between the behaviors found in this model and the dynamics of PV fronts studied in the context of meandering western boundary currents in Earth’s oceans. In addition, the simulations capture the nonlinear aspects of a new feature discovered by the Cassini Visual and Infrared Mapping Spectrometer (VIMS), the String of Pearls, which resides in the equatorward tip of the 47°N jet. The Explicit Planetary Isentropic Coordinate (EPIC) model is used herein.

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Crossref · 10.1175/2010jas3315.1

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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 Sayanagi et al. 2010

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Authors
Sayanagi, K. M., Morales-Juberías, R., & Ingersoll, A. P.
Affiliations
  • California Institute of Technology (US)
  • New Mexico Institute of Mining and Technology (US)
Venue
Journal of the Atmospheric Sciences
Published
2010-08-01
Volume
67
Issue
8
Pages
2658-2678
ISSN
  • 0022-4928 (ISSN-L)
  • 1520-0469
OpenAlex
W2038496891
Cited by
19
References
56
Citations by year
2026: 1 · 2025: 1 · 2023: 1 · 2022: 2 · 2021: 2 · 2020: 1 · 2019: 2 · 2018: 3 · 2015: 1 · 2013: 2 · 2012: 2
FWCI
0.89
Type
journal article
Language
en
Open access
Licence
public-domain
Locations
  • Journal of the Atmospheric Sciences (publishedVersion, public-domain)
  • CaltechAUTHORS (California Institute of Technology) (submittedVersion)
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
jet meandering, shear instability, potential vorticity gradient, western boundary currents, string of pearls

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