Magnetic field morphologies in convective zones influenced by a turbulent surface layer

Open Access

Fig. 11.

(a,b) Components of the mean-field γ-coefficient calculated for N_ρ = 4, $\tilde{Ra} = 32$ $\widetilde{Ra} = 32$ using the method of snapshots (Simard et al. 2016). (a) Radial component, γ_r. (b) Latitudinal component, γ_θ. (c) Total magnetic energy near the surface (r/r_o = 0.9) for run N_ρ = 6, $\tilde{Ra} = 32$ $\widetilde{Ra} = 32$ as a function of spherical harmonic degree l for high- (t_H) and low-energy (t_L) dynamo states.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.