Regimes of thermo-compositional convection and related dynamos in rotating spherical shells

DOI10.1080/03091929.2020.1762875zbMath1482.86037OpenAlexW3024287529WikidataQ114640009 ScholiaQ114640009MaRDI QIDQ5065739

James F. Mather, Radostin D. Simitev

Publication date: 22 March 2022

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

Full work available at URL: http://eprints.gla.ac.uk/214887/1/214887.pdf

zbMATH Keywords

double-diffusive convectiondynamo actionplanetary coresbuoyancy-driven instabilities

Mathematics Subject Classification ID

Geo-electricity and geomagnetism (86A25)

Cites Work

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• Experimental and numerical studies of convection in a rapidly rotating spherical shell
• Zonal flow driven by strongly supercritical convection in rotating spherical shells
• Double-Diffusive Convection at Low Prandtl Number
• Dynamos driven by convection in rotating spherical shells
• Advances in geodynamo modelling
• The onset of thermo-compositional convection in rotating spherical shells
• Planetary Magnetic Fields and Fluid Dynamos
• Double-Diffusive Convection
• Effect of a stabilizing gradient of solute on thermal convection
• Prandtl-number dependence of convection-driven dynamos in rotating spherical fluid shells

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