- Abstract:
-
Numerical simulations of the shallow water equations on rotating spheres produce mixtures of robust vortices and alternating zonal jets, as seen in the atmospheres of the gas giant planets. However, simulations that include Rayleigh friction invariably produce a sub-rotating (retrograde) equatorial jet for Jovian parameter regimes, whilst observations of Jupiter show a super-rotating (prograde) equatorial jet that has persisted over several decades. Super-rotating equatorial jets have recentl...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Accepted manuscript
- Files:
-
-
(x-download, 3.8mb)
-
- Publisher copy:
- 10.1017/jfm.2017.232
-
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- Funding agency for:
- Warneford, ES
- Funding agency for:
- Dellar, P
- Publisher:
- Cambridge University Press Publisher's website
- Journal:
- Journal of Fluid Mechanics Journal website
- Volume:
- 822
- Pages:
- 484-511
- Publication date:
- 2017-06-07
- Acceptance date:
- 2017-04-07
- DOI:
- EISSN:
-
1469-7645
- ISSN:
-
0022-1120
- Pubs id:
-
pubs:700095
- URN:
-
uri:02ecfa66-ecd3-42a5-8093-d8c03753fb45
- UUID:
-
uuid:02ecfa66-ecd3-42a5-8093-d8c03753fb45
- Local pid:
- pubs:700095
- Copyright holder:
- © Cambridge University Press 2017
- Copyright date:
- 2017
- Notes:
- This is the author accepted manuscript following peer review version of the article. The final version is available online from Cambridge University Press at: 10.1017/jfm.2017.232
- License:
- CC BY-NC-ND
Journal article
Super- and sub-rotating equatorial jets in shallow water models of Jovian atmospheres: Newtonian cooling versus Rayleigh friction
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