Saturn atmospheric dynamics one year after Cassini: Long-lived features and time variations in the drift of the Hexagon-Reference-Cited by-同舟云学术

Saturn atmospheric dynamics one year after Cassini: Long-lived features and time variations in the drift of the Hexagon

Published:2020-01 Issue: Volume:336 Page:113429
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Hueso R.,Sánchez-Lavega A.,Rojas J.F.,Simon A.A.,Barry T.,Río-Gaztelurrutia T. del,Antuñano A.,Sayanagi K.M.,Delcroix M.,Fletcher L.N.,García-Melendo E.,Pérez-Hoyos S.,Blalock J.,Colas F.,Gómez-Forrellad J.M.,Gunnarson J.L.,Peach D.,Wong M.H.

Funder

MINECO

Grupos Gobierno Vasco

UPV

Space Telescope Science Institute

Horizon 2020 - Research and Innovation Framework Programme

Generalitat de Catalunya

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference68 articles.

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4. Dynamics of Saturn's polar regions;Antuñano;J. Geophys. Res. Planets,2015

5. Saturn's north polar cyclone and hexagon at depth revealed by Cassini/VIMS;Baines;Planet. Space Sci.,2009

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