The Mars InfraRed Trace Gas Investigation Spectrometer (MIRTIS) for the 2016 Exomars Trace Gas Orbiter

MIRTIS is dual spectrometer aimed at characterizing trace gases in the atmosphere of Mars. It operates in the near- and mid- infrared and shall provide unprecedented sensitivity for the detection of trace gases with geophysical and/or biological origin

Domaines

Astrophysique [astro-ph]

Fichier principal

EPSC2010-546-1.pdf (1.28 Mo)

Origine	Fichiers produits par l'(les) auteur(s)

Florence Henry : Connectez-vous pour contacter le contributeur

https://hal.science/hal-03803606

Soumis le : mardi 29 novembre 2022-13:24:36

Dernière modification le : lundi 2 décembre 2024-14:48:10

Dates et versions

hal-03803606 , version 1 (29-11-2022)

Identifiants

HAL Id : hal-03803606 , version 1
BIBCODE : 2010epsc.conf..546M

Citer

Franck Montmessin, Thierry Fouchet, Florence Henry, Jean-Michel Reess, Pernelle Bernardi, et al.. The Mars InfraRed Trace Gas Investigation Spectrometer (MIRTIS) for the 2016 Exomars Trace Gas Orbiter. European Planetary Science Congress 2010, Sep 2010, Rome, Italy. 5, pp.EPSC2010-546, 2010, EPSC Abstracts. ⟨hal-03803606⟩

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