Near-infrared high-resolution solar spectrum from ACS NIR onboard TGO

Karim Gizatullin (1, 2) , Alexander Trokhimovskiy (1) , Anna Fedorova (1) , Jean-Loup Bertaux (1, 3) , Monique Spite (4) , Alexander Lomakin (1, 2) , Andrey Patrakeev (1) , Franck Montmessin (3) , Oleg Korablev (1)

1 IKI - Space Research Institute of the Russian Academy of Sciences
2 MIPT - Moscow Institute of Physics and Technology [Moscow]
3 PLANETO - LATMOS
4 GEPI - Galaxies, Etoiles, Physique, Instrumentation

The Atmospheric Chemistry Suite (ACS) is Russian contribution to ESA-Roscosmos ExoMars 2016 Trace Gas Orbiter (TGO) mission [1, 2]. It arrived at Mars in October 2016. ACS is a package of three highly sensitive infrared spectrometers with high resolve power (>10,000) and covers from 0.7 to 17µm-the visible to thermal infrared range. In this work, we present results for high-resolution solar spectra observed by ACS NIR instrument in the near-infrared range.

Domains: Solar and Stellar Astrophysics [astro-ph.SR]

Karim Gizatullin, Alexander Trokhimovskiy, Anna Fedorova, Jean-Loup Bertaux, Monique Spite, et al.. Near-infrared high-resolution solar spectrum from ACS NIR onboard TGO. EPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-1786-4. ⟨insu-02292464⟩