Spectrally selective instability of mixed poloidal-toroidal magnetic fields in radiative stellar interiors

Open Access

Fig. 1.

Most unstable eigenmodes for the radial velocity perturbations ${\tilde{u}}_{r}'$ $Mathematical equation: $ \tilde u_r\prime $$ in the unstratified case (δ = 0) at a colatitude of θ = 10° for l = 10 and various azimuthal wavenumbers m. The poloidal-to-toroidal field ratio is μ₀ = 0.1 and μ₀ = 0.2 in the left and right panels, respectively.

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.