A ``stratified spectral model for stable and convective atmospheres
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Publication:1335630
DOI10.1006/jcph.1994.1128zbMath0809.76073OpenAlexW2038857549MaRDI QIDQ1335630
Publication date: 17 October 1994
Published in: Journal of Computational Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1006/jcph.1994.1128
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A semi-implicit spectral method for compressible convection of rotating and density-stratified flows in Cartesian geometry ⋮ Numerical simulation of core convection by a multi-layer semi-implicit spherical spectral method ⋮ Radius ratio dependency of the instability of fully compressible convection in rapidly rotating spherical shells ⋮ Onset of fully compressible convection in a rapidly rotating spherical shell
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