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Possible influence of Martian surface mineralogy on the detectability of atmospheric trace gases - mid-infrared simulation results
DOI: 10.1016/j.pss.2024.105877 Bibcode: 2024P&SS..24905877B

Błęcka, Maria I.

The paper focuses on the influence of the optical properties of Martian surface minerals on remotely detected gaseous components of the Martian atmosphere, when the spectrometer receives a combined signal from the Martian soil and atmosphere. Our considerations are primarily concerned with the detectability of methane, but the problem may also app…

2024 Planetary and Space Science
ExoMars-16 MEx 0
Performance evaluation of pansharpening for planetary exploration: A case study on the implementation of TGO CaSSIS with MRO HiRISE
DOI: 10.1016/j.pss.2024.105997 Bibcode: 2024P&SS..25405997T

Cremonese, G.; Thomas, N.; Re, C. +3 more

The present study analyses the potential of pansharpening algorithms for planetary exploration studies, testing their performance with the 4-band images from the Colour and Stereo Surface Imaging System (CaSSIS) aboard the Exomars 2016 Trace Grace Orbiter (TGO) using HiRISE images from the Mars Reconnaissance Orbiter (MRO) mission as the base. Due…

2024 Planetary and Space Science
ExoMars-16 0
Insights into the interaction between defrosting seasonal ices and gully activity from CaSSIS and HiRISE observations in Sisyphi Cavi, Mars
DOI: 10.1016/j.pss.2023.105743 Bibcode: 2023P&SS..23505743P

Pajola, M.; Munaretto, G.; Vincendon, M. +10 more

Martian gullies are surface features, typically composed of an alcove, a channel and a depositional apron. They have been extensively studied since their first observations in the 2000s and were initially attributed to the action of liquid water. Later studies highlighted that their activity is spatially and temporally correlated with the seasonal…

2023 Planetary and Space Science
ExoMars-16 3
Targeting and image acquisition of Martian surface features with TGO/CaSSIS
DOI: 10.1016/j.pss.2023.105697 Bibcode: 2023P&SS..23105697A

Cremonese, G.; Thomas, N.; Pommerol, A. +12 more

CaSSIS is a high-resolution visual telescope onboard the ExoMars Trace Gas Orbiter. The mission started the primary science phase in April 2018. The relatively small single image footprint (typically 40 km × 9.5 km) when compared to the total surface area of Mars demands that images should be targeted and target selection is key for the science re…

2023 Planetary and Space Science
ExoMars-16 2
Preface for special issue on the Colour and Stereo Surface Imaging System (CaSSIS) at Mars
DOI: 10.1016/j.pss.2023.105753 Bibcode: 2023P&SS..23605753S

Sefton-Nash, Elliot; Wilson, Colin; Hauber, Ernst +2 more

The Colour and Stereo Surface Imaging System (CaSSIS) is the main camera on board the ExoMars Trace Gas Orbiter (TGO). Following launch of TGO on 14 March 2016, CaSSIS began nominal science operations in April 2018. At the time of writing CaSSIS has acquired an average of 21 observations per day, totaling 20.5 Tbits of downlinked telemetry, and ha…

2023 Planetary and Space Science
ExoMars-16 0
Calibration of NOMAD on ESA's ExoMars Trace Gas Orbiter: Part 1 - The Solar Occultation channel
DOI: 10.1016/j.pss.2021.105411 Bibcode: 2022P&SS..21805411T

Vandaele, Ann Carine; Neefs, Eddy; Aoki, Shohei +17 more

Nadir and Occultation for MArs Discovery (NOMAD) is a 3-channel spectrometer suite that is currently orbiting Mars onboard ESA's ExoMars Trace Gas Orbiter, measuring the composition of the Martian atmosphere in unprecedented detail. Of the three channels, two operate in the infrared: the Solar Occultation (SO) channel observes gas species in the 2…

2022 Planetary and Space Science
ExoMars-16 11
Calibration of the NOMAD-UVIS data
DOI: 10.1016/j.pss.2022.105504 Bibcode: 2022P&SS..21805504W

Vandaele, Ann Carine; Neefs, Eddy; Aoki, Shohei +23 more

The Ultraviolet and VIsible Spectrometer (UVIS), covering the 200-650 nm range, is one of three spectrometers that comprise the NOMAD instrument on the ExoMars 2016 Trace Gas Orbiter (TGO). UVIS can operate in solar occultation, nadir and limb viewing mode and was designed to monitor ozone and aerosols in the Martian atmosphere. Here, we describe …

2022 Planetary and Space Science
ExoMars-16 10
Multiband photometry of Martian Recurring Slope Lineae (RSL) and dust-removed features at Horowitz crater, Mars from TGO/CaSSIS color observations
DOI: 10.1016/j.pss.2022.105443 Bibcode: 2022P&SS..21405443M

Pajola, M.; Cremonese, G.; Thomas, N. +12 more

Recurring Slope Lineae (RSL) are narrow, dark streaks typically lengthening down Martian steep slopes during warm seasons, fading during the cold ones and regularly recurring every Martian year. Their origin is still debated. Although initially interpreted as possible flows of seeping water, either coming from a subsurface aquifer or through atmos…

2022 Planetary and Space Science
ExoMars-16 10
Water vapor saturation and ice cloud occurrence in the atmosphere of Mars
DOI: 10.1016/j.pss.2021.105390 Bibcode: 2022P&SS..21205390P

Vandaele, Ann Carine; Aoki, Shohei; Kleinböhl, Armin +3 more

We investigate water vapor saturation in the martian atmosphere in the presence or proximity of water ice clouds. We evaluate mixing ratio profiles of ambient water vapor derived from measurements by the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) and the Nadir and Occultation for MArs Discovery (NOMAD) instrument in comparison wi…

2022 Planetary and Space Science
ExoMars-16 10
Absolute calibration of the Colour and Stereo Surface Imaging System (CaSSIS)
DOI: 10.1016/j.pss.2021.105394 Bibcode: 2022P&SS..21105394T

Almeida, Miguel; Cremonese, Gabriele; Thomas, Nicolas +5 more

The Colour and Stereo Surface Imaging System (CaSSIS) onboard the ExoMars Trace Gas Orbiter (TGO) has observed several standard stars and Jupiter with the aim of deriving the absolute calibration factors that convert observed signal into reflectance ("I over F"). The targets were observed through all four colour filters and hence a relative calibr…

2022 Planetary and Space Science
ExoMars-16 9