A planetary-scale disturbance in a long living three vortex coupled system in Saturn's atmosphere
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A system of subpolar vortices at latitudes 60-65°N has been present at least since 2011.
“A system of subpolar vortices at latitudes 60-65 ◦ N present at least since 2011.”
From Saturn atmospheric dynamics one year after Cassini: Long-lived features and time variations in the drift of the Hexagon (2020) · cites this paper as del R´ ıo-Gaztelurrutia et al., 2018
del R ́ ıo-Gaztelurrutia et al. (2018) studied with similar observations the onset and evolution of a large polar perturbation caused by the interaction of a system of subpolar vortices.
“del R´ ıo-Gaztelurrutia et al. (2018) studied with similar observations the onset and evolution of a large polar perturbation caused by the interaction of a system of subpolar vortices.”
From Saturn atmospheric dynamics one year after Cassini: Long-lived features and time variations in the drift of the Hexagon (2020) · cites this paper as del R´ ıo-Gaztelurrutia et al., 2018
The perturbation was the consequence of the interaction of a system of three vortices located at 65° N (ACA) with the dark vortex at 60° N.
“The perturbation was the consequence of the interaction of a system of three vortices located at 65 ◦ N and named ACA after Anticyclone-Cyclone-Anticyclone with the dark vortex at 60 ◦ N (del R´ ıo-Gaztelurrutia et al., 2018).”
From Saturn atmospheric dynamics one year after Cassini: Long-lived features and time variations in the drift of the Hexagon (2020) · cites this paper as del R´ ıo-Gaztelurrutia et al., 2018
This spot is possibly the vortex labelled 'A1' in Cassini ISS images during Grand Finale and is the subpolar single vortex described by del Río-Gaztelurrutia et al. (2018).
“This spot is possibly the vortex labelled as 'A1' in the high-resolution Cassini ISS images obtained during Cassini's Grand Finale (Figure 1 in Ingersoll et al. 2018) and is the subpolar single vortex described by del R´ ıo-Gaztelurrutia et al. (2018).”
From Saturn atmospheric dynamics one year after Cassini: Long-lived features and time variations in the drift of the Hexagon (2020) · cites this paper as del R´ ıo-Gaztelurrutia et al. (2018)
The ACA system's track in 2013-2015 exhibited oscillations in longitude with an amplitude of ~10° and period of ~8.2 months with respect to a single linear fit.
“According to del R´ ıo-Gaztelurrutia et al. (2018), the track of the ACA system in the period 2013-2015 exhibited oscillations in longitude with an amplitude of ∼ 10 ◦ and period of ∼ 8 . 2 months with respect to a single linear fit”
From Saturn atmospheric dynamics one year after Cassini: Long-lived features and time variations in the drift of the Hexagon (2020) · cites this paper as del R´ ıo-Gaztelurrutia et al. (2018)
The ACA system at 64° N was first observed in Cassini ISS images in 2011.
“The ACA system at 64 ◦ N was first observed in Cassini ISS images in 2011 (del R´ ıo-Gaztelurrutia et al., 2018).”
From Saturn atmospheric dynamics one year after Cassini: Long-lived features and time variations in the drift of the Hexagon (2020) · cites this paper as del R´ ıo-Gaztelurrutia et al., 2018
The ACA system's oscillations increased at the time of the 2015 polar perturbation, reaching a maximum amplitude of nearly 20°.
“These oscillations were accurately observed on Cassini ISS images and increased at the time of the 2015 polar perturbation reaching their maximum amplitude (nearly 20 ◦ ).”
From Saturn atmospheric dynamics one year after Cassini: Long-lived features and time variations in the drift of the Hexagon (2020) · cites this paper as del R´ ıo-Gaztelurrutia et al. (2018)
This vortex was one of the vortices implied in a polar perturbation that developed in Saturn in May-July 2015.
“This vortex was one of the vortices implied in a polar perturbation that developed in Saturn in May-July 2015.”
From Saturn atmospheric dynamics one year after Cassini: Long-lived features and time variations in the drift of the Hexagon (2020) · cites this paper as del R´ ıo-Gaztelurrutia et al., 2018
The interactions they experienced in 2015 that resulted in a subpolar planetary scale perturbation have not developed again.
“The interactions they experienced in 2015 that resulted in a subpolar planetary scale perturbation (del R´ ıoGaztelurrutia et al., 2018) has not developed again.”
From Saturn atmospheric dynamics one year after Cassini: Long-lived features and time variations in the drift of the Hexagon (2020) · cites this paper as del R´ ıo-Gaztelurrutia et al., 2018
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Self-citationSaturn's Atmosphere in Northern Summer Revealed by JWST/MIRI
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“This spot is possibly the vortex labelled as “A1” in the high-resolution Cassini ISS images obtained during Cassini’s Grand Finale (Figure 1 in Ingersoll et al. 2018) and is the subpolar single vortex described by del Ŕıo-Gaztelurrutia et al. (2018).”
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Self-citationDynamics and clouds in planetary atmospheres from telescopic observations
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Self-citationSaturn's atmosphere at 1–10 kilometer resolution
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“The wavenumber k is now 2π divided by the jet spacing, which is about 6200 km according to Figure 1 of del Rio-Gaztelurrutia et al. (2018), and the velocity from which the kinetic energy is computed is still 20 m s 1.”
BackgroundInfluentialMidsummer Atmospheric Changes in Saturn’s Northern Hemisphere from the Hubble OPAL Program
Simon, A. A., Hueso, R., Sánchez-Lavega, A., & Wong, M. H. (2021) · The Planetary Science Journal · doi:10.3847/psj/abe40f · Cited by 8 · see citing works
“These include subpolar vortexes at 60°–65° N (del Río-Gaztelurrutia et al. 2018) and a remnant anticyclonic vortex at 42° N (near 50° W longitude in 2018) from the 2010–2011 Great White Storm (Sánchez-Lavega et al. 2012; Sayanagi et al. 2013; Fletcher et al. 2017).”
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Multiple convective storms within a single cyclone on Saturn
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Self-citationInteraction of Saturn’s Hexagon With Convective Storms
Sánchez-Lavega, A., Garcia‐Melendo, E., del Río-Gaztelurrutia, T., Hueso, R., Simon, A. A., Wong, M. H., Ahrens‐Velásquez, K., Sòria, M., Barry, T., Go, C., et al. (2021) · Geophysical Research Letters · doi:10.1029/2021gl092461 · Cited by 3 · see citing works
Self-citationGlobal climate modelling of Saturn’s atmosphere, Part V: Large-scale vortices
Donnelly, P. T., Spiga, A., Guerlet, S., James, M. K., & Bardet, D. (2024) · Icarus · doi:10.1016/j.icarus.2024.116302 · Cited by 1 · see citing works
The Dynamics of the Atmosphere of Saturn
Sánchez-Lavega, A. (2026) · doi:10.1093/9780197851500.003.0342
Self-citation
- Authors
- del Río-Gaztelurrutia, T., Sánchez-Lavega, A., Antuñano, A., Legarreta, J., García-Melendo, E., Sayanagi, K. M., Hueso, R., Wong, M. H., Pérez-Hoyos, S., Rojas, J. F., Simon, A. A., de Pater, I., Blalock, J., & Barry, T.
- Affiliations
- University of the Basque Country (ES)
- Hampton University (US)
- University of California, Berkeley (US)
- Goddard Space Flight Center (US)
- ORCID
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 2018-03
- Volume
- 302
- Pages
- 499-513
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W2774446149
- Cited by
- 16
- References
- 53
- Citations by year
- 2026: 1 · 2024: 1 · 2023: 2 · 2022: 2 · 2021: 3 · 2020: 1 · 2019: 5 · 2018: 1
- FWCI
- 1.05
- Type
- journal article
- Language
- en
- Open access
- green
- hdl.handle.net
- Licence
- cc-by-nc-nd
- www.elsevier.com/tdm/userlicense/1.0/ (tdm)
- Locations
- Icarus (publishedVersion)
- RECERCAT (Consorci de Serveis Universitaris de Catalunya) (acceptedVersion, cc-by-nc-nd)
- UPCommons institutional repository (Universitat Politècnica de Catalunya) (acceptedVersion, cc-by-nc-nd)
- Communities in ADDI (University of the Basque Country) (submittedVersion, cc-by-nc-nd)
- LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) (submittedVersion, cc-by-nc-nd)
- Hispana (submittedVersion, cc-by-nc-nd)
- RECERCAT (Consorci de Serveis Universitaris de Catalunya) (submittedVersion, cc-by-nc-nd)
- Funders
- Spanish MICIIN (AYA2015-65041-P)
- Grupos Gobierno Vasco (IT-765-13, UFI11/55)
- UPV/EHU
- NASA Cassini Data Analysis (NNX15AD33G, NNX15AD34G)
- 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
- Saturn, vortex interaction, zonal wind profiles, vortex drift, relative vorticity, cloud advection, vortex stability, nonlinear simulation, upper troposphere, static stability, wind shear
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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