Hadley circulations and Kelvin wave–driven equatorial jets in the atmospheres of Jupiter and Saturn.
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Shallow-flow models that posit differential radiative heating as the driver of the flow can generate equatorial superrotation, but they require artifices such as additional equatorial heat or wave sources that have no clear physical interpretation.
“Similarly, shallow-flow models that posit differential radiative heating as the driver of the flow can generate equatorial superrotation, but they require artifices such as additional equatorial heat or wave sources that have no clear physical interpretation (e.g., Williams 2003a,b;Yamazaki et al. 2005;Lian and Showman 2008).”
From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Yamazaki et al. 2005
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NUMERICAL SIMULATIONS OF ATMOSPHERIC DYNAMICS ON THE GIANT PLANETS
Lian, Y. (2009) · UA Campus Repository (The University of Arizona)
- Authors
- Yamazaki, Y. H., Read, P. L., & Skeet, D. R.
- Affiliations
- University of Oxford (GB)
- ORCID
- Read, P.L.
- Venue
- Planetary and Space Science
- Publisher
- Elsevier BV
- Published
- 2005-04
- Volume
- 53
- Issue
- 5
- Pages
- 508-525
- ISSN
- 0032-0633 (ISSN-L)
- OpenAlex
- W2030836652
- Cited by
- 28
- References
- 55
- Citations by year
- 2024: 1 · 2023: 1 · 2022: 1 · 2021: 2 · 2020: 3 · 2019: 1 · 2018: 2 · 2016: 1 · 2015: 1 · 2013: 1 · 2012: 1
- FWCI
- 1.36
- Type
- journal article
- Language
- en
- Open access
- green
- doi.org
- Locations
- Planetary and Space Science (publishedVersion)
- Newcastle University ePrints (Newcastle Univesity)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Ionosphere and magnetosphere dynamics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- Hadley circulation, Kelvin waves, equatorial jet, superrotation, Jupiter, Saturn, meridional circulation, momentum transfer, global climate models, primitive equations, planetary atmospheres
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