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A Complex Storm System in Saturn's North Polar Atmosphere in 2018Saturn’s convective storms usually fall in two categories. One consists of mid-sized storms ~ 2,000 km wide, appearing as irregular bright cloud systems that evolve rapidly, on scales of a few days. The other includes the exceptional Great White Spots (GWS), planetary-scale giant storms that disturb a full latitude band, and which have been observed only seven times. Here we report a new intermediate type, observed in 2018 in the North Polar Region. Four large storms (the first one lasting longer than 200 days) formed sequentially in close latitudes, experiencing mutual encounters, and leading to zonal disturbances affecting a full latitude band ~ 8,000 km wide, during at least 8 months. Dynamical simulations indicate that each storm required energies ~ 100 times smaller than those necessary for a GWS. This event occurred at about the same latitude and season as the GWS in 1960, in close correspondence with the cycle of approximately 60 years hypothesized for equatorial GWSs.
Document ID
20190034077
Acquisition Source
Goddard Space Flight Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
A Sánchez-Lavega ORCID
(Universidad del Pais Vasco Bilbao, Spain)
E García-Melendo
(Universitat Politècnica de Catalunya Barcelona, Spain)
J Legarreta
(Universidad del Pais Vasco Bilbao, Spain)
R Hueso ORCID
(Universidad del Pais Vasco Bilbao, Spain)
T del Río-Gaztelurrutia
(Universidad del Pais Vasco Bilbao, Spain)
J F Sanz-Requena
(Universidad Europea Miguel de Cervantes Valladolid, Spain)
S Pérez-Hoyos ORCID
(Universidad del Pais Vasco Bilbao, Spain)
A A Simon ORCID
(Goddard Space Flight Center Greenbelt, Maryland, United States)
M H Wong
(University of California, Berkeley Berkeley, California, United States)
M Soria
(Universitat Politècnica de Catalunya Barcelona, Spain)
J M Gómez-Forrellad
(Fabra Observatory Barcelona, Spain)
T Barry
(Broken Hill Observatory Broken Hill, New South Wales, Australia)
M Delcroix ORCID
(Societe Astronomique de France Paris, France)
K M Sayanagi
(Hampton University Hampton, Virginia, United States)
J J Blalock ORCID
(Hampton University Hampton, Virginia, United States)
J L Gunnarson
(Hampton University Hampton, Virginia, United States)
U Dyudina
(California Institute of Technology Pasadena, California, United States)
S Ewald ORCID
(California Institute of Technology Pasadena, California, United States)
Date Acquired
December 23, 2019
Publication Date
October 21, 2019
Publication Information
Publication: Nature Astronomy
Publisher: Nature Research
Volume: 4
Issue Publication Date: February 1, 2020
e-ISSN: 2397-3366
URL: https://www.nature.com/articles/s41550-019-0914-9
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
GSFC-E-DAA-TN74574
Funding Number(s)
PROJECT: AYA2015-65041-P
CONTRACT_GRANT: NAS5-26555
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
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