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The Colour and Stereo Surface Imaging System (CaSSIS) for the ExoMars Trace Gas Orbiter
DOI: 10.1007/s11214-017-0421-1 Bibcode: 2017SSRv..212.1897T

Mangold, N.; Hansen, C. J.; Cremonese, G. +58 more

The Colour and Stereo Surface Imaging System (CaSSIS) is the main imaging system onboard the European Space Agency's ExoMars Trace Gas Orbiter (TGO) which was launched on 14 March 2016. CaSSIS is intended to acquire moderately high resolution (4.6 m/pixel) targeted images of Mars at a rate of 10-20 images per day from a roughly circular orbit 400 …

2017 Space Science Reviews
ExoMars-16 118
Retrieving cloud, dust and ozone abundances in the Martian atmosphere using SPICAM/UV nadir spectra
DOI: 10.1016/j.pss.2017.04.011 Bibcode: 2017P&SS..142....9W

Vandaele, A. C.; Montmessin, F.; Willame, Y. +4 more

We present the retrieval algorithm developed to analyse nadir spectra from SPICAM/UV aboard Mars-Express. The purpose is to retrieve simultaneously several parameters of the Martian atmosphere and surface: the dust optical depth, the ozone total column, the cloud opacity and the surface albedo. The retrieval code couples the use of an existing com…

2017 Planetary and Space Science
ExoMars-16 MEx 43
NOMAD spectrometer on the ExoMars trace gas orbiter mission: part 2—design, manufacturing, and testing of the ultraviolet and visible channel
DOI: 10.1364/ao.56.002771 Bibcode: 2017ApOpt..56.2771P

Vandaele, Ann Carine; Neefs, Eddy; Ristic, Bojan +48 more

2017 Applied Optics
ExoMars-16 43
Boulder abundances and size-frequency distributions on Oxia Planum-Mars: Scientific implications for the 2020 ESA ExoMars rover
DOI: 10.1016/j.icarus.2017.05.011 Bibcode: 2017Icar..296...73P

Quantin, Cathy; Pajola, Maurizio; Carter, John +4 more

This paper presents the abundances and the size-frequency distributions (SFD) of boulders identified on a sector of the prime landing site for the ExoMars 2020 rover, in Oxia Planum region. By means of a HiRISE image, boulders ≥ 1.75 m across have been identified and subdivided according to the two main Oxia Planum geological units: the Noachian c…

2017 Icarus
ExoMars-16 MEx 31
Measurement of dust optical depth using the solar irradiance sensor (SIS) onboard the ExoMars 2016 EDM
DOI: 10.1016/j.pss.2017.01.015 Bibcode: 2017P&SS..138...33T

Rannou, P.; Toledo, D.; Gómez, L. +5 more

The solar irradiance sensor (SIS) was included in the DREAMS package onboard the ExoMars 2016 Entry Descent and Landing Demonstrator Module, and has been selected in the METEO meteorological station onboard the ExoMars 2020 Lander. This instrument is designed to measure at different time intervals the scattered flux or the sum of direct flux and s…

2017 Planetary and Space Science
ExoMars-16 16
On the link between martian total ozone and potential vorticity
DOI: 10.1016/j.icarus.2016.10.004 Bibcode: 2017Icar..282..104H

Holmes, James A.; Lewis, Stephen R.; Patel, Manish R.

We demonstrate for the first time that total ozone in the martian atmosphere is highly correlated with the dynamical tracer, potential vorticity, under certain conditions. The degree of correlation is investigated using a Mars global circulation model including a photochemical model. Potential vorticity is the quantity of choice to explore the dyn…

2017 Icarus
ExoMars-16 13
A deep search for the release of volcanic gases on Mars using ground-based high-resolution infrared and submillimeter spectroscopy: Sensitive upper limits for OCS and SO2
DOI: 10.1016/j.icarus.2017.05.014 Bibcode: 2017Icar..296....1K

Villanueva, G. L.; Mumma, M. J.; Tokunaga, A. T. +1 more

Recent volcanic activity has long been considered a distinct possibility that would place major constraints on the evolution of Mars' interior. Volcanic activity would result in the outgassing of sulfur-bearing species. As part of our multi-band search for active release of volcanic gases on Mars, we looked for carbonyl sulfide (OCS) at its combin…

2017 Icarus
ExoMars-16 13
Diurnal variation in martian dust devil activity
DOI: 10.1016/j.icarus.2017.01.003 Bibcode: 2017Icar..292..154C

Lewis, S. R.; Chapman, R. M.; Balme, M. +1 more

We show that the dust devil parameterisation in use in most Mars Global Circulation Models (MGCMs) results in an unexpectedly high level of dust devil activity during morning hours.

Prior expectations of the diurnal variation of Martian dust devils are based mainly upon the observed behaviour of terrestrial dust devils: i.e. that the majority…

2017 Icarus
ExoMars-16 MEx 12
DREAMS-SIS: The Solar Irradiance Sensor on-board the ExoMars 2016 lander
DOI: 10.1016/j.asr.2017.04.002 Bibcode: 2017AdSpR..60..103A

Toledo, D.; Gómez, L.; Apéstigue, V. +10 more

The Solar Irradiance Sensor (SIS) was part of the DREAMS (Dust characterization, Risk assessment, and Environment Analyzer on the Martian Surface) payload package on board the ExoMars 2016 Entry and Descent Module (EDM), "Schiaparelli". DREAMS was a meteorological station aimed at the measurement of several atmospheric parameters, as well as the p…

2017 Advances in Space Research
ExoMars-16 12
Signatures of the Martian rotation parameters in the Doppler and range observables
DOI: 10.1016/j.pss.2017.05.008 Bibcode: 2017P&SS..144...74Y

Yseboodt, Marie; Dehant, Véronique; Péters, Marie-Julie

The position of a Martian lander is affected by different aspects of Mars' rotational motions: the nutations, the precession, the length-of-day variations and the polar motion. These various motions have a different signature in a Doppler observable between the Earth and a lander on Mars' surface. Knowing the correlations between these signatures …

2017 Planetary and Space Science
ExoMars-16 12