Loïc Rossi
Publications
Publications
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Stratigraphic and Isotopic Evolution of the Martian Polar Caps from Paleo-Climate Models8th International Conference on Mars Polar Science and Exploration, Jul 2024, Whitehorse, Yukon, Canada. pp.LPI Contribution No. 3064, 2024, id.6037 |
Hydrogen Escape in Current and Past MarsSeventh edition of the Spanish Meeting of Planetary Sciences and Exploration of the Solar System (7th CPESS), Jul 2023, Valladolid (Spain), Spain. pp.id.80590 |
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Simulation of deuterium and hydrogen loss on Mars by thermal, photochemical and solar wind processes55th Annual Meeting of the Division for Planetary Sciences, Oct 2023, San Antonio (TX), United States |
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Modeling the Martian HDO cycle with a Global Climate Model during the “dusty” seasonEuroplanet Science Congress 2022, Sep 2022, Granada, Spain. pp.EPSC2022-451, ⟨10.5194/epsc2022-451⟩ |
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Simulation of the H Escape Variability with a Global Climate ModelSeventh international workshop on the Mars atmosphere: Modelling and observations, Jun 2022, Paris, France. pp.id.3104 |
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Measurements of HDO and the D/H ratio in the Martian atmosphere from ACS MIREuroplanet Science Congress 2022, Sep 2022, Granada, Spain. pp.EPSC2022-696 |
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Challenges in Mars Climate Modelling with the LMD Mars Global Climate Model, Now Called the Mars “Planetary Climate Model” (PCM)Seventh international workshop on the Mars atmosphere: Modelling and observations, Jun 2022, Paris, France. pp.id.1102 |
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Simulation of the atomic deuterium density and escape at Mars and comparison with MAVEN/IUVS observationsEuroplanet Science Congress 2022, Sep 2022, Grenade, Spain. pp.EPSC2022-568, ⟨10.5194/epsc2022-568⟩ |
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Climatological controls on the chemical stratigraphy of the martian polar layer depositsSeventh International Workshop on the Mars Atmosphere: Modelling and Observations, Jun 2022, Paris, France |
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Modeling the HDO Cycle with a Global Climate Model During the MY34 "Dusty" SeasonSeventh International Workshop on the Mars Atmosphere: Modelling and Observations, Jun 2022, Paris, France. pp.id.2406 |
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Simulation of the Hydrogen escape from Mars using a Global Climate ModelEuroplanet Science Congress 2022, Sep 2022, Granada, Spain. pp.EPSC2022-693, ⟨10.5194/epsc2022-693⟩ |
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Modelling the HDO cycle of the Martian atmosphere with the LMD Global Climate ModelEuropean Planetary Science Congress. EPSC 2021, Sep 2021, Virtual Meeting, France. ⟨10.5194/epsc2021-296⟩ |
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Comparison of the HDO cycle in the LMD Mars GCM with ACS/TGO observationsEuropean Planetary Science Congress. EPSC 2021, Sep 2021, virtual Meeting, France. ⟨10.5194/epsc2021-281⟩ |
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Escape of water from Mars: study with a ground-to-exosphere global modelEuropean Planetary Science Congress. EPSC 2021, Sep 2021, Virtual Meeting, Germany. ⟨10.5194/epsc2021-395⟩ |
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Modeling the HDO cycle with the LMD Mars GCMEuroplanet Science Congress 2020, Sep 2020, Online, Unknown Region. pp.EPSC2020-680, ⟨10.5194/epsc2020-680⟩ |
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Modeling of the effect of the MY34 Global Dust Storm on the martian HDO cycle.Europlanet Science Congress 2020, Sep 2020, Virtual Meeting, Unknown Region. pp.EPSC2020-626, ⟨10.5194/epsc2020-626⟩ |
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Modeling of HDO in the Martian atmosphere22nd EGU General Assembly, May 2020, Online, Unknown Region. pp.id.8565, ⟨10.5194/egusphere-egu2020-8565⟩ |
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Vertical distributions of CO, H<sub>2</sub>O, HDO, and temperature in the atmosphere of Mars after a year of observations with the ExoMars Trace Gas Orbiter (TGO) Atmospheric Chemistry Suite mid-infrared (ACS MIR) solar occultation spectrometerEPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-1463-3 |
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Modeling of HDO in the Martian atmosphereEPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-1372 |
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Exploring HDO and H 2 O on Mars with the ACS instrument onboard TGOEuropean Planetary Science Congress 2018, Sep 2018, Berlin, Germany. pp.EPSC2018-472-2 |
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Modeling of HDO in the Martian atmosphereEuropean Planetary Science Congress 2018, Sep 2018, Berlin, Germany. pp.EPSC2018-786 |
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Latitudinal and temporal variability of Venus clouds and hazes observed by polarimetry with SPICAV-IRInternational Venus Conference 2016, Apr 2016, Oxford, United Kingdom |
The Clouds of Venus – an overview of Venus Express resultsEuropean Planetary Science Congress 2015, Sep 2015, Nantes, France. pp.EPSC2015-762-1 |
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Retrieval of Venus' clouds and hazes properties with polarimetric data from SPICAV/VExEuropean Planetary Science Congress 2015, Sep 2015, Nantes, France. pp.EPSC2015-119 |
Study of Venus cloud layers with polarimetric data from SPICAV/VExEGU General Assembly 2014, Apr 2014, Vienna, Austria |
Simulation of the atomic deuterium density and escape at Mars and comparison with MAVEN/IUVS observationsSeventh international workshop on the Mars atmosphere: Modelling and observations, Jun 2022, Paris, France. pp.id.3552 |
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Study of Venus cloud layers by polarimetry using SPICAV/VExEGU General Assembly 2015, Apr 2015, Vienna, Austria. pp.EGU2015-1656 |
Study of Venus cloud layers by polarimetry using SPICAV/VExAstronomical Polarimetry 2014, May 2014, Grenoble, France. , 2014 |
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Study of Venus' cloud layers by polarimetry using SPICAV/VExEGU General Assembly 2013, Apr 2013, Vienna, Austria. 15, pp.2013 - 3110, 2013 |
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Study of Venus cloud layers by polarimetry using SPICAV/VExInternational Venus Workshop, Jun 2013, Catania, Italy. , 2013 |
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Ultraviolet Spectropolarimetry as a Tool for Understanding the Diversity of Exoplanetary Atmospheres. Astro2020 Science White Paper2019 |
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Ariel: Enabling planetary science across light-years[Research Report] ESA/SCI(2020)1, European Space Agency. 2021, 147 p |
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Étude des nuages de Vénus par polarimétrie avec les données de l’instrument SPICAV-IR à bord de Venus ExpressPlanétologie et astrophysique de la terre [astro-ph.EP]. Université de Versailles-Saint Quentin en Yvelines, 2015. Français. ⟨NNT : 2015VERS041V⟩ |