Fig. 2
Download original image
Spectrum of semi-diurnal atmospheric thermal tides. Plotted is the imaginary part of the normalized pressure anomaly (
; Eq. (22)) as a function of the normalized forcing frequency ω = (Ω − n⋆)/n⋆ = σ/2n⋆, where n⋆ is the mean motion of the stellar perturber. The planetary-stellar parameters are those of the fiducial planetary system defined in Sect. 3.1.
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.