Back to Search Start Over

ACS experiment for atmospheric studies on 'ExoMars-2016' Orbiter

Authors :
Anna Fedorova
Alexei Grigoriev
Nikolai Ignatiev
Alexander Trokhimovskiy
K. A. Anufreichik
Franck Montmessin
Oleg Korablev
Alexei Shakun
T. O. Kozlova
Moscow Institute of Physics and Technology [Moscow] (MIPT)
Space Research Institute of the Russian Academy of Sciences (IKI)
Russian Academy of Sciences [Moscow] (RAS)
PLANETO - LATMOS
Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Source :
Astronomicheskii Vestnik / Solar System Research, Astronomicheskii Vestnik / Solar System Research, MAIK Nauka/Interperiodica, 2015, 49 (7), pp.529-537. ⟨10.1134/S003809461507014X⟩, Astronomicheskii Vestnik / Solar System Research, 2015, 49 (7), pp.529-537. ⟨10.1134/S003809461507014X⟩
Publication Year :
2015
Publisher :
Pleiades Publishing Ltd, 2015.

Abstract

International audience; ACS is a set of spectrometers for atmospheric studies (Atmospheric Chemistry Suite). It is one of the Russian instruments for the Trace Gas Orbiter (TGO) of the Russian-European “ExoMars” program. The purpose of the experiment is to study the Martian atmosphere by means of two observations regimes: sensitive trace gases measurements in solar occultations and by monitoring the atmospheric state during nadir observations. The experiment will allow us to approach global problems of Mars research such as current volcanism, and the modern climate status and its evolution. Also, the experiment is intended to solve the mystery of methane presence in the Martian atmosphere. Spectrometers of the ACS set cover the spectral range from the near IR-range (0.7 μm) to the thermal IR-range (17 μm) with spectral resolution λ/Δλ reaching 50000. The ACS instrument consists of three independent IR spectrometers and an electronics module, all integrated in a single unit with common mechanical, electrical and thermal interfaces. The article gives an overview of scientific tasks and presents the concept of the experiment.

Details

ISSN :
16083423 and 00380946
Volume :
49
Database :
OpenAIRE
Journal :
Solar System Research
Accession number :
edsair.doi.dedup.....46e4ba46908e99cc0428cb346495d358
Full Text :
https://doi.org/10.1134/s003809461507014x