Fig. 7
Atmospheric temperature in the UMLT of Venus. A) Dayside temperatures inferred from CO2 NLTE nadir spectra taken by VEx/VIRTIS-H; B) dayside temperatures from the VTGCM by Brecht & Bougher (2012) and averaged for the pressure interval 10-2–10-5 mb; C) difference between temperatures from the VTGCM and VIRTIS-H; D) nightside temperatures inferred with stellar radio-occultation data from VEx/SPICAV (Piccialli et al. 2015) and averaged for the pressure interval 10-2–10-5 mb.
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.