Projects
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The NOMAD instrument onboard the ExoMars 2016 Trace Gas Orbiter is in orbit around Mars.
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2031: Radiative transfer in planetary atmospheres of celestial bodies, including (exo)planets and moons
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2031: Spectrometer onboard of ESA’s EnVision mission to Venus. It aims at mapping the atmosphere near the surface and above the cloud deck.
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2029: Characterization of the detectors and expected performances of the Moons and Jupiter Imaging Spectrometer (MAJIS) onboard JUICE
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2027: Venus Atmosphere exploration through Machine learning and Open Science in preparation to EnVision
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2027: Assessment of key minor species Detections in the Atmosphere of MarS measured by NOMAD/TGO
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2025: Mesoscale Modelling for ExoMars TGO/NOMAD To Understand gravity waves in the Martian atmosphere
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ASIMUT is a modular program for radiative transfer calculations in planetary atmospheres. It is one of our main tool.
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2021: Understanding relationships and interactions between different planetary reservoirs and their evolution through time.
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2020: Spectroscopy and forward model error improvement for CH4 retrieval in the TIR.
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2018: Five grand science themes which challenge our current understanding of the complex couplings of the Mars climate.
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2017: PLANET TOPERS stands for Planets, Tracing the Transfer, Origin, Preservation, and Evolution of their ReservoirS.
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2016: Stands for European Unified Research on Observations of Venus using coordinated Space- and Earth-based Facilities.
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2016: Visualization and sharing of Mars data to strength collaborative science data analysis and real-time operations.
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2015: High resolution microwave, infrared and Raman molecular spectroscopy for atmospheric, planetological and astrophysical applications.
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2015: Collaboration with the Indian Space Research Organisation interested in our experience in radiative transfer models for Mars.
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2014: Synergetic retrieval algorithms for near-surface concentrations of CH4 and CO from passive remote sensing measurements.
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2014: The Solar Occultation in the Infrared instrument SOIR delivered high spectral resolution spectra of the Venus' mesosphere.
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In 2013, 3 International Teams have been selected to deal with Venus related issues:
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International Mars Architecture for the Return of Samples, under the umbrella of the International Mars Exploration Working Group.
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Spectroscopic Investigation of the Characteristics of the Atmosphere of Mars onboard Mars Express
