Constraining the depth of Saturn's zonal winds by measuring thermal and gravitational signals
Based on straightforward dynamical considerations, we show how available and upcoming measurements of Saturn's thermal and gravitational signals can be used to constrain the depth to which its zonal winds penetrate. The dynamical considerations issue from the facts that Saturn has a strong intr...
Главные авторы: | Liu, J, Schneider, T, Fletcher, L |
---|---|
Формат: | Journal article |
Язык: | English |
Опубликовано: |
Academic Press Inc.
2014
|
Схожие документы
-
CHANGES TO SATURN'S ZONAL-MEAN TROPOSPHERIC THERMAL STRUCTURE AFTER THE 2010-2011 NORTHERN HEMISPHERE STORM
по: Achterberg, R, и др.
Опубликовано: (2014) -
Mapping potential vorticity dynamics on Saturn: Zonal mean circulation from Cassini and Voyager data
по: Read, P, и др.
Опубликовано: (2009) -
Equatorial winds on Saturn and the stratospheric oscillation
по: Li, L, и др.
Опубликовано: (2011) -
A chorus of the winds-on Saturn!
по: Read, P
Опубликовано: (2018) -
Energy exchanges in Saturn's polar regions from Cassini observations: Eddy-zonal flow interactions
по: Read, PL, и др.
Опубликовано: (2022)