Numerical simulation of core convection by a multi-layer semi-implicit spherical spectral method

DOI10.1016/j.jcp.2011.08.014zbMath1242.85005OpenAlexW2002134861MaRDI QIDQ422498

Tao Cai, Licai Deng, Kwing L. Chan

Publication date: 18 May 2012

Published in: Journal of Computational Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.jcp.2011.08.014

zbMATH Keywords

turbulencecore convectionmulti-layer schemesolar corespherical spectral method

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Computational methods for problems pertaining to astronomy and astrophysics (85-08) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (5)

A semi-implicit spectral method for compressible convection of rotating and density-stratified flows in Cartesian geometry ⋮ Radius ratio dependency of the instability of fully compressible convection in rapidly rotating spherical shells ⋮ Curvilinear grids for WENO methods in astrophysical simulations ⋮ Radial collocation methods for the onset of convection in rotating spheres ⋮ Onset of fully compressible convection in a rapidly rotating spherical shell

Uses Software

• ASH

Cites Work

• A ``stratified spectral model for stable and convective atmospheres
• Computational aspects of a code to study rotating turbulent convection in spherical shells
• The stratified approximation for computing geophysical flows
• A staggered spectral element model with application to the oceanic shallow water equations
• Rotating convection in f‐boxes: Faster rotation

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