Energy exchanges in Saturn's polar regions from Cassini observations: Eddy-zonal flow interactions
Saturn's polar regions (polewards of ∼63° planetocentric latitude) are strongly dynamically active with zonal jets, polar cyclones and the intriguing north polar hexagon (NPH) wave. Here we analyze measurements of horizontal winds, previously obtained from Cassini images by Antuñano et al. (201...
المؤلفون الرئيسيون: | Read, PL, Antunano, A, Cabanes, S, Colyer, G, Gaztelurrutia, TDR, Sanchez-Lavega, A |
---|---|
التنسيق: | Journal article |
اللغة: | English |
منشور في: |
Wiley
2022
|
مواد مشابهة
-
Cassini Saturn polar velocity fields
حسب: Antuñano, A, وآخرون
منشور في: (2021) -
Potential vorticity of Saturn's polar regions: seasonality and instabilities
حسب: Antuñano, A, وآخرون
منشور في: (2019) -
Mapping potential vorticity dynamics on Saturn: Zonal mean circulation from Cassini and Voyager data
حسب: Read, P, وآخرون
منشور في: (2009) -
Multilayer hazes over Saturn’s hexagon from Cassini ISS limb images
حسب: A. Sánchez-Lavega, وآخرون
منشور في: (2020-05-01) -
Haze and cloud structure of Saturn's North Pole and Hexagon Wave from Cassini/ISS imaging
حسب: Sanz-Requena, J, وآخرون
منشور في: (2017)