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Elsevier, Planetary and Space Science, (119), p. 233-249

DOI: 10.1016/j.pss.2015.10.003

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Science objectives and performances of NOMAD, a spectrometer suite for the ExoMars TGO mission

Journal article published in 2015 by Mike Wolff, Jose-Jeronimo Zafra, Ann Carine Vandaele, Eddy Neefs, G. Bellucci, D. Bellucci, Rachel Drummond, Jose-Juan Lopez-Moreno ORCID, I. R. Thomas, Giancarlo Bellucci, J. Vanderauwera, Frank Daerden, Manish Patel, Mark Allen, J.-J. Lopez-Moreno and other authors.
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

The NOMAD spectrometer suite on the ExoMars Trace Gas Orbiter will map the composition and distribution of Mars' atmospheric trace species in unprecedented detail, fulfilling many of the scientific objectives of the joint ESA-Roscosmos ExoMars Trace Gas Orbiter mission. The instrument is a combination of three channels, covering a spectral range from the UV to the IR, and can perform solar occultation, nadir and limb observations. In this paper, we present the science objectives of the instrument and how these objectives have influenced the design of the channels. We also discuss the expected performance of the instrument in terms of coverage and detection sensitivity.