Calibration of NOMAD on ESA's ExoMars Trace Gas Orbiter: Part 2 - The Limb, Nadir and Occultation (LNO) channel - INSU - Institut national des sciences de l'Univers Access content directly
Journal Articles Planetary and Space Science Year : 2022

Calibration of NOMAD on ESA's ExoMars Trace Gas Orbiter: Part 2 - The Limb, Nadir and Occultation (LNO) channel

Ian R. Thomas
  • Function : Author
Shohei Aoki
  • Function : Author
Loïc Trompet
  • Function : Author
Séverine Robert
  • Function : Author
Cédric Depiesse
  • Function : Author
Yannick Willame
  • Function : Author
Justin T. Erwin
  • Function : Author
Ann Carine Vandaele
  • Function : Author
Frank Daerden
  • Function : Author
Arnaud Mahieux
  • Function : Author
Eddy Neefs
  • Function : Author
Bojan Ristic
  • Function : Author
Laszlo Hetey
  • Function : Author
Sophie Berkenbosch
  • Function : Author
Roland Clairquin
  • Function : Author
Bram Beeckman
  • Function : Author
Manish R. Patel
  • Function : Author
Jose Juan Lopez-Moreno
  • Function : Author
Giancarlo Bellucci
  • Function : Author

Abstract

The Nadir and Occultation for MArs Discovery (NOMAD) instrument is a 3-channel spectrometer suite on the ESA ExoMars Trace Gas Orbiter. Since April 2018, when the nominal science mission began, it has been measuring the constituents of the Martian atmosphere. NOMAD contains three separate spectrometers, two of which operate in the infrared: the Solar Occultation (SO) channel makes only solar occultation observations, and therefore has the best resolving power (∼20,000) and a wider spectral region covering 2.2-4.3 μm. The Limb, Nadir and Occultation (LNO) channel covers the 2.2-3.8 μm spectral region and can operate in limb, nadir or solar occultation pointing modes. The Ultraviolet-VISible (UVIS) channel operates in the UV-visible region, from 200 to 650 nm, and can measure in limb, nadir or solar occultation modes like LNO.

The LNO channel has a lower resolving power (∼10,000) than the SO channel, but is still typically an order of magnitude better than previous instruments orbiting Mars. The channel primarily operates in nadir-viewing mode, pointing directly down to the surface to measure the narrow atmospheric molecular absorption lines, clouds and surface features in the reflected sunlight. From the depth and position of the observed atmospheric absorption lines, the constituents of the Martian atmosphere and their column densities can be derived, leading to new insights into the processes that govern their distribution and transport. Surface properties can also be derived from nadir observations by observing the shape of the spectral continuum.

Many calibration measurements were made prior to launch, on the voyage to Mars, and continue to be made in-flight during the science phase of the mission. This work, part 2, addresses the aspects of the LNO channel calibration that are not covered elsewhere, namely: the LNO ground calibration setup, the LNO occultation and nadir boresight pointing vectors, LNO detector characterisation and nadir/limb illumination pattern, instrument temperature effects, and finally the radiometric calibration of the LNO channel. An accompanying paper, part 1 (Thomas et al., 2021, this issue), addresses similar aspects for SO, the other infrared channel in NOMAD. A further accompanying paper (Cruz-Mermy et al., 2021, this issue) investigated the LNO radiometric calibration in more detail, approaching the work from a theoretical perspective. The two calibrations agree with each other to within 3%, validating each calibration method.

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insu-03745276 , version 1 (04-08-2022)

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Ian R. Thomas, Shohei Aoki, Loïc Trompet, Séverine Robert, Cédric Depiesse, et al.. Calibration of NOMAD on ESA's ExoMars Trace Gas Orbiter: Part 2 - The Limb, Nadir and Occultation (LNO) channel. Planetary and Space Science, 2022, 218, ⟨10.1016/j.pss.2021.105410⟩. ⟨insu-03745276⟩
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