Monitoring of the atmosphere of Mars with ACS TIRVIM nadir observations on ExoMars TGO - INSU - Institut national des sciences de l'Univers Accéder directement au contenu
Communication Dans Un Congrès Année : 2018

Monitoring of the atmosphere of Mars with ACS TIRVIM nadir observations on ExoMars TGO

Franck Montmessin

Résumé

The ExoMars Trace Gas Orbiter (TGO), a mission by ESA and Roscosmos started its operational scientific phase in March 2018. The Atmospheric Chemistry Suite (ACS) is a set of three spectrometers (NIR, MIR, and TIRVIM) designed to observe the Martian atmosphere in solar occultation, nadir and limb geometry [1]. The thermal infrared channel-TIRVIM is a Fourier-transform spectrometer encompassing the spectral range of 1.7-17 μm, with the best spectral resolution 0.13 cm-1. In nadir operation mode, the primary goal of TIRVIM is the long-term monitoring of atmospheric temperature and aerosol (dust and ice clouds) state from the surface to approximately 60 km. We present the results of the first half year operation in orbit around Mars.
Fichier principal
Vignette du fichier
EPSC2018-891-1.pdf (165.35 Ko) Télécharger le fichier
Origine : Fichiers produits par l'(les) auteur(s)

Dates et versions

insu-04451750 , version 1 (11-02-2024)

Identifiants

Citer

Nikolay Ignatiev, Alexey Grigoriev, Alexey Shakun, Boris Moshkin, Dmitry Patsaev, et al.. Monitoring of the atmosphere of Mars with ACS TIRVIM nadir observations on ExoMars TGO. European Planetary Science Congress 2018, Sep 2018, Berlin, Germany. pp.EPSC2018-891-1. ⟨insu-04451750⟩
46 Consultations
8 Téléchargements

Partager

Gmail Facebook X LinkedIn More