Marginal stability of planetary convection

Computer Science

Scientific paper

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Scientific paper

Review of the known and recent researches is presented for the onset of Boussinesq convection in rapidly rotating spherical shell imitating the planetary interiors. Those researches and the first principles of well-mixed compositional and/or almost adiabatic thermal non-Boussinesq convection in the planets allow deriving new results for marginal convection stability and planetary magnetic field excitation.

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