A 1D radiative-convective model for the atmospheres of hot terrestrial planets.
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Updated
May 28, 2024 - Fortran
A 1D radiative-convective model for the atmospheres of hot terrestrial planets.
A shallow water model coded on the sphere. Licensed under the MIT license.
Normal Modes at Planetary Scales
MagIC is a high-performance code that solves the magneto-hydrodynamics equations in rotating spherical shells
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