Free Access

Fig. 9

image

Mean density and velocity structure in the hydrodynamic simulation of the atmosphere of WASP-8 b. The density is depicted by the dashed line and the velocity by the dash-dotted one. The atmospheric layer where the bulk EUV emission is absorbed is marked by a circle. The triangles mark the radii, where the atmosphere becomes collisionless for neutral hydrogen and protons. The arrow marks the sonic point and the plus sign the Roche lobe size. Oscillations are visible in the velocity structure of the lower atmosphere. The hydrodynamic simulation is only valid below the exobase at 3Rpl. This planet hosts a stable and compact thermosphere.

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.