Abstract: First Numerical Simulations of Turbulent Dynamos Driven by Libration, Precession and Tides in Triaxial Ellipsoids - An Alternative Route for Planetary Magnetism (2017 AGU Fall Meeting)

First Numerical Simulations of Turbulent Dynamos Driven by Libration, Precession and Tides in Triaxial Ellipsoids - An Alternative Route for Planetary Magnetism

Michael Le Bars, Sandeep R. Kanuganti and Benjamin Favier, CNRS, Aix Marseille Univ, Centrale Marseille, IRPHE UMR 7342, Marseille, France

Back to: Planetary Magnetism and Gravity I