Deep two-dimensional turbulence: An idealized model for atmospheric jets of the giant outer planets
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Publication:3081177
DOI10.1080/03091920412331336398zbMath1206.85012OpenAlexW2065376813MaRDI QIDQ3081177
Jun-Ichi Yano, Pierre Drossart, Olivier Talagrand
Publication date: 5 March 2011
Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1080/03091920412331336398
Related Items (2)
On magnetostrophic inertia-less waves in quasi-geostrophic models of planetary cores ⋮ Physical interpretation of spiralling-columnar convection in a rapidly rotating annulus with radial propagation properties of Rossby waves
Cites Work
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- Deep Convection in the Interior of Major Planets: A Review
- Emergence of intense jets and Jupiter's Great Red Spot as maximum-entropy structures
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