2D Studies of Various Approximations Used for Modeling Convection in Giant Planets

DOI10.1080/03091920410001696126zbMath1206.85005OpenAlexW2157252991MaRDI QIDQ3080169

Martha Evonuk, Gary A. Glatzmaier

Publication date: 5 March 2011

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1080/03091920410001696126

zbMATH Keywords

numerical modelinggiant plants

Mathematics Subject Classification ID

Planetary atmospheres (85A20) Computational methods for problems pertaining to astronomy and astrophysics (85-08)

Related Items (4)

Quasi-geostrophic approximation of anelastic convection ⋮ Centrifugally driven compressible convection ⋮ Linear theory of compressible convection in rapidly rotating spherical shells, using the anelastic approximation ⋮ Large eddy simulations of two-dimensional turbulent convection in a density-stratified fluid

Cites Work

• Numerical modeling of magnetohydrodynamic convection in a rapidly rotating spherical shell: Weak and strong field dynamo action
• Convection in an imposed magnetic field. Part 1. The development of nonlinear convection
• Convection in an imposed magnetic field. Part 2. The dynamical regime
• Rapidly rotating turbulent Rayleigh-Bénard convection
• Zonal flow driven by strongly supercritical convection in rotating spherical shells
• Rayleigh number scaling in numerical convection

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