Vertical damping of gravity waves evaluated from ACS-TGO solar occultation measurements on Mars

The dataset represents results on gravity wave (GW) activity and damping in the atmosphere of Mars for the 3.5 Martian years (second half of MY34 - end of MY37) obtained by the middle infrared (MIR) and near infrared (NIR) spectrometers of the Atmospheric Chemistry Suite (ACS) operating on board ExoMars Trace Gas Orbiter in solar occultation mode. The dataset represents the digitized figures of the article Starichenko et al. (2025) "Vertical damping of gravity waves evaluated from ACS-TGO solar occultation measurements on Mars".