Dynamics of Y dwarf atmospheres | Astronomy & Astrophysics (A&A)

Open Access

Fig. 4

Vertical mixing profiles of all simulations. The T–p profile is overplotted with the convective mixing K_zz and the advective mixing contribution $H (z) \sqrt{{〈 w^{2} (z) 〉}_{h}}$ $Mathematical equation: $H(z)\sqrt {{{\left\langle {{w^2}(z)} \right\rangle }_h}} $$ . The pressure extents of convective regions are shown as gray horizontal bands in each panel.

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.