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Jupiter’s overturning circulation: Breaking waves take the place of solid boundaries

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journal contribution
posted on 2021-12-01, 10:33 authored by Andrew P Ingersoll, Sushil Atreya, Scott J Bolton, Shawn Brueshaber, Leigh N Fletcher, Steven M Levin, Cheng Li, Liming Li, Jonathan I Lunine, Glenn S Orton, Hunter Waite
Cloud-tracked wind observations document the role of eddies in putting momentum into the zonal jets. Chemical tracers, lightning, clouds, and temperature anomalies document the rising and sinking in the belts and zones, but questions remain about what drives the flow between the belts and zones. We suggest an additional role for the eddies, which is to generate waves that propagate both up and down from the cloud layer. When the waves break they deposit momentum and thereby replace the friction forces at solid boundaries that enable overturning circulations on terrestrial planets. By depositing momentum of one sign within the cloud layer and momentum of the opposite sign above and below the clouds, the eddies maintain all components of the circulation, including the stacked, oppositely rotating cells between each belt-zone pair, and the zonal jets themselves.

Plain Language Summary
The dark belts and bright zones that circle the planet at constant latitude, along with the jet streams on the belt-zone boundaries, are the iconic dynamical features of Jupiter's atmosphere. But the circulation cells with rising, sinking, and cross-latitude motion are just as important because they maintain the storms and turbulent eddies. Voyager and Cassini have shown that the turbulent eddies put energy into the jet streams. We argue that the eddies also put energy into the circulation cells. They do this by generating waves that break as they propagate above and below the clouds. The breaking waves provide the essential forces that replace those that occur on planets with solid boundaries.

Funding

National Aeronautic and Space Administration (NASA). Grant Number: 80NSSC20K0555.

NASA, Jet Propulsion Laboratory (JPL). Grant Number: 80NM0018D0004

Heising-Simons Foundation (HSF). Grant Number: 51 Peg b postdoctoral

Juno Project of NASA

EC, H2020, H2020 Priority Excellent Science, H2020 European Research Council (ERC). Grant Number: 723890

History

Citation

Geophysical Research Letters, 48 (23), 2021, e2021GL095756. https://doi.org/10.1029/2021GL095756

Author affiliation

School of Physics and Astronomy

Version

  • VoR (Version of Record)

Published in

Geophysical Research Letters

Volume

48

Issue

23

Publisher

American Geophysical Union (AGU)

issn

0094-8276

eissn

1944-8007

Acceptance date

2021-10-25

Copyright date

2021

Available date

2021-12-01

Notes

This article is a companion to Duer et al. (2021), https://doi.org/10.1029/2021GL095651.

Language

en

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