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Slantwise convection on fluid planets

Published:2016-10-28 Issue:20 Volume:43 Page:10,611-10,620
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

O'Neill Morgan E¹,Kaspi Yohai¹

Affiliation:

1. Department of Earth and Planetary Sciences; Weizmann Institute of Science; Rehovot Israel

Funder

Israeli Ministry of Science

Federal German Ministry of Education and Research

Weizmann Institute of Science (WIS) Helen Kimmel Center for Planetary Science

WIS Dean's Postdoctoral Fellowship

WIS Postdoctoral Koshland Prize

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2016GL071188/fullpdf

Reference55 articles.

1. Zero potential vorticity envelopes for the zonal-mean velocity of the Venus/Titan atmospheres;Allison;J. Atmos. Sci.,1994

2. Richardson number constraints for the Jupiter and outer planet wind regime;Allison;Geophys. Res. Lett.,1995

3. A similarity model for the windy Jovian thermocline;Allison;Planet. Space Sci.,2000

4. Galileo probe Doppler residuals as the wave-dynamical signature of weakly stable, downward-increasing stratification in Jupiter's deep wind layer;Allison;Geophys. Res. Lett.,2001

5. Deep winds on Jupiter as measured by the Galileo probe;Atkinson;Nature,1997

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