A Four Martian Years Climatology of the Vertical Properties of Martian Water Ice Clouds with TGO/ACS-MIR

The ACS-MIR_profiles_reff_kext folder contains the retrieved water ice clouds effective radii (reff) along with the atmospheric extinction (kext) at 3.2μm and 3.4μm below the haze top, retrieved from TGO/ACS-MIR observations acquired between Ls=163° (MY 34) and Ls=265° (MY 38). The complete list of the processed observations with their coordinates is provided in ACS-MIR_coord_profiles_2026-08-10.csv. The Mars_PCM_profiles folder contains profiles of the atmospheric properties predicted by the Mars PCM version 6 at the coordinates of the TGO/ACS-MIR observations from MY 34 to MY 37.