ON THE MODE OF DYNAMO ACTION IN A GLOBAL LARGE-EDDY SIMULATION OF SOLAR CONVECTION

146 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

CYCLIC MAGNETIC ACTIVITY DUE TO TURBULENT CONVECTION IN SPHERICAL WEDGE GEOMETRY (2012, methodology): “Later, oscillatory solutions have been obtained from similar simulations with subgrid-scale modeling (Ghizaru et al. 2010; Racine et al. 2011).”
Solar Dynamo Theory (2014, methodology): “…with angular velocity isocontours approximately aligned with the rotational axis, but now it is a pole-to-equator angular velocity difference markedly smaller than solar (cf. Käpylä et al. 2010, their figure 1; Brown et al. 2011, their figure 3c; and Racine et al. 2011, their figure 4).”
MAGNETIC WREATHS AND CYCLES IN CONVECTIVE DYNAMOS (2012, methodology): “Further work by Racine et al. (2011) has interpreted these results in terms of mean-field dynamo theory.”