Fig. C.1

Imaginary part of the surface pressure variation created by the semidiurnal thermal tide as a function of the normalized tidal frequency
for a Venus-sized planet of surface pressure ps = 10 bar and orbital radius a = aVenus. Results obtained using GCM simulations are designated by points. Spectra are plotted for two cases: the reference case of the study, where the atmosphere is mainly composed of
N2 (black line), and the case treated in Appendix C, where the atmosphere is composed of CO2 with a mixture of water vapour and sulphuric acid.
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