Jupiter's Overturning Circulation: Breaking Waves Take the Place of Solid Boundaries
Abstract
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.
Additional Information
© 2021. The Authors. This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited. Issue Online: 28 November 2021; Version of Record online: 28 November 2021; Accepted manuscript online: 25 October 2021; Manuscript accepted: 12 October 2021; Manuscript revised: 06 October 2021; Manuscript received: 04 June 2021. One portion of this research was carried out at the California Institute of Technology under a contract with the National Aeronautics and Space Administration (NASA), Grant/Cooperative Agreement Number 80NSSC20K0555. Another portion of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004). C. L. was supported by the 51 peg b Postdoctoral Fellowship sponsored by the Heising-Simons foundation. L. N. F. was supported by EC |H2020 |H2020 Priority Excellent Science |H2020 European Research Council (ERC) (723890). Other authors acknowledge support from the Juno Project of NASA. Data Availability Statement: Juno MWR data used in producing Figure 2 are available through the Planetary Atmospheres Node of the Planetary Data System (https://pds-atmospheres.nmsu.edu/cgi-bin/getdir.pl?&volume=jnomwr_1100). Analyzed data are published in Oyafuso et al. (2020).Attached Files
Published - 2021GL095756.pdf
Supplemental Material - 2021gl095756-sup-0001-supporting_information_si-s01.pdf
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Additional details
- Eprint ID
- 112135
- Resolver ID
- CaltechAUTHORS:20211201-165438995
- NASA
- 80NSSC20K0555
- NASA/JPL/Caltech
- 80NM0018D0004
- Heising-Simons Foundation
- 51 Pegasi b Fellowship
- European Research Council (ERC)
- 723890
- Created
-
2021-12-01Created from EPrint's datestamp field
- Updated
-
2021-12-01Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)