Spherical convective dynamos in the rapidly rotating asymptotic regime
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DOI: 10.1017/jfm.2016.789
Abstract: Self-sustained convective dynamos in planetary systems operate in an asymptotic regime of rapid rotation, where a balance is thought to hold between the Coriolis, pressure, buoyancy and Lorentz forces (the MAC balance). Classical numerical solutions… read more here.
Keywords: spherical convective; asymptotic regime; mac balance; convective dynamos ... See more keywords