Fig. 2.
Meridional flow system for two models for a star with a mass of M = 0.60 M⊙ and a rotation period of 1 day (top panels) and 10 days (bottom panels). Left panel: isocontours of the stream function. We find poleward circulation at the top of the convection zone (blue full line) and equatorward flow at the base of the convection zone (red dashed line).
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.