Projects
- Details
ISSI team on intercomparison on MAVEN-TGO CO2 density and temperature with comparisons to general circulation models too.
- Details
The NOMAD instrument onboard the ExoMars 2016 Trace Gas Orbiter is in orbit around Mars.
- Details
2031: Radiative transfer in planetary atmospheres of celestial bodies, including (exo)planets and moons
- Details
2031: Spectrometer onboard of ESA’s EnVision mission to Venus. It aims at mapping the atmosphere near the surface and above the cloud deck.
- Details
2029: Characterization of the detectors and expected performances of the Moons and Jupiter Imaging Spectrometer (MAJIS) onboard JUICE
- Details
2027: Venus Atmosphere exploration through Machine learning and Open Science in preparation to EnVision
- Details
2027: Assessment of key minor species Detections in the Atmosphere of MarS measured by NOMAD/TGO
- Details
2025: Mesoscale Modelling for ExoMars TGO/NOMAD To Understand gravity waves in the Martian atmosphere
- Details
ASIMUT is a modular program for radiative transfer calculations in planetary atmospheres. It is one of our main tool.
- Details
2024: Mars and the IsotopiC Ratio Of water: Budget and Evolution
Although Mars is now a cold, dry, and inhospitable planet, a wealth of evidence indicates that it was once much wetter and may have supported liquid water on its surface billions of years ago. Understanding how Mars lost most of its water is essential for reconstructing its climate history and assessing its past habitability. This project combined observations from recent Mars missions with advanced modeling efforts to investigate the evolution of water and its isotopes (H₂O and HDO) from the subsurface to the upper atmosphere. By studying the processes controlling isotopic fractionation and atmospheric escape, the project provided new insights into the mechanisms driving water loss on Mars and helped constrain the planet’s past water inventory and long-term evolution.
- Details
2021: Understanding relationships and interactions between different planetary reservoirs and their evolution through time.
- Details
2020: Spectroscopy and forward model error improvement for CH4 retrieval in the TIR.
- Details
2018: Five grand science themes which challenge our current understanding of the complex couplings of the Mars climate.
- Details
2017: PLANET TOPERS stands for Planets, Tracing the Transfer, Origin, Preservation, and Evolution of their ReservoirS.
- Details
2016: Stands for European Unified Research on Observations of Venus using coordinated Space- and Earth-based Facilities.
- Details
2016: Visualization and sharing of Mars data to strength collaborative science data analysis and real-time operations.
- Details
2015: High resolution microwave, infrared and Raman molecular spectroscopy for atmospheric, planetological and astrophysical applications.
- Details
2015: Collaboration with the Indian Space Research Organisation interested in our experience in radiative transfer models for Mars.
- Details
2014: Synergetic retrieval algorithms for near-surface concentrations of CH4 and CO from passive remote sensing measurements.
- Details
2014: The Solar Occultation in the Infrared instrument SOIR delivered high spectral resolution spectra of the Venus' mesosphere.
- Details
In 2013, 3 International Teams have been selected to deal with Venus related issues:
- Details
International Mars Architecture for the Return of Samples, under the umbrella of the International Mars Exploration Working Group.
- Details
Spectroscopic Investigation of the Characteristics of the Atmosphere of Mars onboard Mars Express
