Vertical structure of tropospheric winds on gas giants

Abstract Zonal mean zonal velocity profiles from cloud‐tracking observations on Jupiter and Saturn are used to infer latitudinal variations of potential temperature consistent with a shear stable potential vorticity distribution. Immediately below the cloud tops, density stratification is weaker on...

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Main Authors: R. K. Scott, T. J. Dunkerton
Format: Article
Language:English
Published: Wiley 2017-04-01
Series:Geophysical Research Letters
Subjects:
Online Access:https://doi.org/10.1002/2017GL072628
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author R. K. Scott
T. J. Dunkerton
author_facet R. K. Scott
T. J. Dunkerton
author_sort R. K. Scott
collection DOAJ
description Abstract Zonal mean zonal velocity profiles from cloud‐tracking observations on Jupiter and Saturn are used to infer latitudinal variations of potential temperature consistent with a shear stable potential vorticity distribution. Immediately below the cloud tops, density stratification is weaker on the poleward and stronger on the equatorward flanks of midlatitude jets, while at greater depth the opposite relation holds. Thermal wind balance then yields the associated vertical shears of midlatitude jets in an altitude range bounded above by the cloud tops and bounded below by the level where the latitudinal gradient of static stability changes sign. The inferred vertical shear below the cloud tops is consistent with existing thermal profiling of the upper troposphere. The sense of the associated mean meridional circulation in the upper troposphere is discussed, and expected magnitudes are given based on existing estimates of the radiative timescale on each planet.
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spelling doaj-art-1069c9da1a1f43a79d6fa762dcc13b2e2025-08-20T03:10:24ZengWileyGeophysical Research Letters0094-82761944-80072017-04-014473073308110.1002/2017GL072628Vertical structure of tropospheric winds on gas giantsR. K. Scott0T. J. Dunkerton1School of Mathematics and Statistics University of St Andrews St Andrews UKNorthWest Research Associates Seattle Washington USAAbstract Zonal mean zonal velocity profiles from cloud‐tracking observations on Jupiter and Saturn are used to infer latitudinal variations of potential temperature consistent with a shear stable potential vorticity distribution. Immediately below the cloud tops, density stratification is weaker on the poleward and stronger on the equatorward flanks of midlatitude jets, while at greater depth the opposite relation holds. Thermal wind balance then yields the associated vertical shears of midlatitude jets in an altitude range bounded above by the cloud tops and bounded below by the level where the latitudinal gradient of static stability changes sign. The inferred vertical shear below the cloud tops is consistent with existing thermal profiling of the upper troposphere. The sense of the associated mean meridional circulation in the upper troposphere is discussed, and expected magnitudes are given based on existing estimates of the radiative timescale on each planet.https://doi.org/10.1002/2017GL072628zonal jetspotential vorticitygas giant planetsvertical shearstability
spellingShingle R. K. Scott
T. J. Dunkerton
Vertical structure of tropospheric winds on gas giants
Geophysical Research Letters
zonal jets
potential vorticity
gas giant planets
vertical shear
stability
title Vertical structure of tropospheric winds on gas giants
title_full Vertical structure of tropospheric winds on gas giants
title_fullStr Vertical structure of tropospheric winds on gas giants
title_full_unstemmed Vertical structure of tropospheric winds on gas giants
title_short Vertical structure of tropospheric winds on gas giants
title_sort vertical structure of tropospheric winds on gas giants
topic zonal jets
potential vorticity
gas giant planets
vertical shear
stability
url https://doi.org/10.1002/2017GL072628
work_keys_str_mv AT rkscott verticalstructureoftroposphericwindsongasgiants
AT tjdunkerton verticalstructureoftroposphericwindsongasgiants