HIGHLIGHTS
SUMMARY
WOLFF ET AL. Water ice clouds are recognized to have a fundamental contribution to the Martian atmosphere through their formation processes and their roles in the atmospheric radiation budget (e_g, Clancy et_al, 2017; Wolff et_al, 2019; and references within). EMIRS can explicitly distinguish between water-ice and dust aerosols, while analysis of EXI data must adopt a dust column. Comparison to Global Climate Models A fundamental motivation for the EXI cloud retrievals is the creation of products that characterize the diurnal cycle to constrain MGCMs (Almatroushi et_al, 2021; Amiri et_al, 2022). Combining EXI with . . .
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