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Communication Dans Un Congrès Année : 2019

Temperature distribution in Mars atmosphere as measured by the ACS-MIR/ExoMars-TGO solar occultations

Résumé

We report results from the first year of temperature distribution retrievals in Mars atmosphere from the solar occultation measurements, being performed by the Atmospheric Chemistry Suite (ACS) onboard the ExoMars Trace Gas Orbiter (TGO). Statistics of observations provides almost regular time coverage including the beginning of the Martian global dust storm in June 2018 (LS≈190, MY34). Temperature variability before and during the storm is studied at altitudes from 3-30 km up to 80-100 km.
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insu-04450667 , version 1 (10-02-2024)

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Denis Belyaev, Anna Fedorova, Alexander Trokhimovskiy, Oleg Korablev, Franck Montmessin, et al.. Temperature distribution in Mars atmosphere as measured by the ACS-MIR/ExoMars-TGO solar occultations. EPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-1566-1. ⟨insu-04450667⟩
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