Trace gas observations by ACS MIR onboard ExoMars/TGO

Alexander Trokhimovski 1 Anna Fedorova 1 Oleg Korablev 1 Andrey Patrakeev 1 Nikita Kokonkov 1 Alexey Shakun 1 Franck Montmessin 2 Franck Lefèvre 2
1 IKI - Space Research Institute of the Russian Academy of Sciences
2 IMPEC - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
Abstract : The Atmospheric Chemistry Suite (ACS) package is a part of Russian contribution to ExoMars 2016 Trace Gas Orbiter (TGO) ESA-Roscosmos mission for studies of the Martian atmosphere and climate [1]. The design of the middle infrared (MIR) channel was optimized to overachieve the primary science goal of the TGO mission by accomplishing the most sensitive measurements ever of the trace gases present in the Martian atmosphere. Having both, high spectral resolution and signal to noise ratio (SNR) of acquired spectra, ACS MIR channel operates in solar occultation in the spectral range of 2.3-4.24 μm.
Document type :
Conference papers
Complete list of metadatas

Cited literature [10 references]  Display  Hide  Download
https://hal-insu.archives-ouvertes.fr/insu-02306414
Contributor : Catherine Cardon <>
Submitted on : Saturday, October 5, 2019 - 1:09:11 PM
Last modification on : Friday, January 10, 2020 - 3:42:35 PM

File

EPSC-DPS2019-1603-1.pdf
Publisher files allowed on an open archive

Identifiers

  • HAL Id : insu-02306414, version 1

Collections

INSU | LATMOS | UVSQ | CNRS | SORBONNE-UNIVERSITE | SU-SCIENCES | UNIV-PARIS-SACLAY

Citation

Alexander Trokhimovski, Anna Fedorova, Oleg Korablev, Andrey Patrakeev, Nikita Kokonkov, et al.. Trace gas observations by ACS MIR onboard ExoMars/TGO. EPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-1603-1. ⟨insu-02306414⟩

Export

BibTeX TEI DC DCterms EndNote

Share

Metrics

Record views

23

Files downloads

12

Contact

Informations

CCSD