Optical and radiometric models of the NOMAD instrument Part I: The UVIS channel

NOMAD Team

Research output: Contribution to journalArticle

15 Citations (Scopus)

Abstract

The NOMAD instrument has been designed to best fulfil the science objectives of the ExoMars Trace Gas Orbiter mission that will be launched in 2016. The instrument is a combination of three channels that cover the UV, visible and IR spectral ranges and can perform solar occultation, nadir and limb observations. In this series of two papers, we present the optical models representing the three channels of the instrument and use them to determine signal to noise levels for different observation modes and Martian conditions. In this first part, we focus on the UVIS channel, which will sound the Martian atmosphere using nadir and solar occultation viewing modes, covering the 200-650nm spectral range. High SNR levels (>1000) can easily be reached for wavelengths higher than 300nm both in solar occultation and nadir modes when considering binning. Below 300nm SNR are lower primarily because of the lower signal and the impact of atmospheric absorption.

Original languageEnglish
Pages (from-to)30028-30042
Number of pages15
JournalOptics Express
Volume23
Issue number23
DOIs
Publication statusPublished - 2015 Nov 16

ASJC Scopus subject areas

  • Atomic and Molecular Physics, and Optics

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