Published August 10, 2026
| Version v1
Dataset
Open
A Four Martian Years Climatology of the Vertical Properties of Martian Water Ice Clouds with TGO/ACS-MIR
Authors/Creators
- 1. Institut de Recherche en Astrophysique et Planétologie (IRAP)
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2.
Laboratoire atmosphères, milieux, observations spatiales
Description
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.