Emmanuel MARCQ
Publications
Publications
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3D Monte-Carlo modeling of Venus' reflectance in UVEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. ⟨10.5194/epsc-dps2025-403⟩ |
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Goals and Structure of Envision’s VenSpec Ground-Based Observations Working GroupEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. ⟨10.5194/epsc-dps2025-477⟩ |
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Synergistic Observations of Venus’ Surface and Atmosphere: The Role of VenSpec on the ESA EnVision MissionEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. ⟨10.5194/epsc-dps2025-1409⟩ |
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From Core to Clouds: Laboratory Synergy within the EnVision’s VenSpec Science TeamEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. ⟨10.5194/epsc-dps2025-1787⟩ |
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3D Monte Carlo Radiative Transfer for Parameter Retrieval in Planetary AtmospheresEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. pp.EPSC-DPS2025-681, ⟨10.5194/epsc-dps2025-681⟩ |
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Multiple temporal and spatial scales variation of sulfur dioxide at the Venusian cloud-topEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. ⟨10.5194/epsc-dps2025-1141⟩ |
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Observability of small scale atmospheric spatial variability by the VenSpec-U instrument onboard EnVisionEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. ⟨10.5194/epsc-dps2025-1481⟩ |
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VenSpec-H spectrometer on the ESA EnVision mission: Instrument’s statusEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. ⟨10.5194/epsc-dps2025-1652⟩ |
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Water and sulfur dioxide thermal mapping on Venus : Long-term monitoring and vertical distribution of SO2 within and above the cloudsEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. ⟨10.5194/epsc-dps2025-366⟩ |
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Mapping Venus in Emissivity: The Venus Emissivity Mapper, VenSpec-M on EnVision and VEM on VERITAS missions to VenusEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. ⟨10.5194/epsc-dps2025-991⟩ |
The Venus Emissivity Mapper (VEM): instrument science performance requirements derived from VERITAS and EnVisionInfrared Remote Sensing and Instrumentation XXXIII. Proceedings SPIE Volume 136120G, SPIE, Aug 2025, San Diego, United States. ⟨10.1117/12.3064436⟩ |
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Detecting volcanic ash of eruption plumes on Venus by imaging in the near infrared windowsEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. ⟨10.5194/epsc-dps2025-1485⟩ |
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Defining Surface Targets for the EnVision’s VenSpec Suite: Collaborative Strategies of the Regions of Interest Working GroupEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. ⟨10.5194/epsc-dps2025-1653⟩ |
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Prospective Venus Cloud trace species detectability as inferred from HubbleEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. ⟨10.5194/epsc-dps2025-1266⟩ |
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VenSpec Radiative Transfer Modeling Working GroupEPSC-DPS Joint Meeting 2025, Sep 2025, Helsinki, Finland. ⟨10.5194/epsc-dps2025-1645⟩ |
The VenSpec suite organization: collaborative development from instrument proposal to scientific analysisInfrared Remote Sensing and Instrumentation XXXII. Proceedings SPIE volume 13144, SPIE, Aug 2024, San Diego, United States. ⟨10.1117/12.3027459⟩ |
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Scientific objectives and instrumental requirements of the IR spectrometer VenSpec-H onboard EnVisionInfrared Remote Sensing and Instrumentation XXXII. Proceedings SPIE 13144, Aug 2024, San Diego, United States. 16 p., ⟨10.1117/12.3027948⟩ |
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The VenSpec-U spectrometer onboard EnVision: sensitivity studiesInfrared Remote Sensing and Instrumentation XXXII. Proceedings SPIE 13144, Aug 2024, San Diego, United States. 43 p., ⟨10.1117/12.3027500⟩ |
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A spherical and heterogeneous radiative transfer code for near-infrared remote sensing: application to TitanEuroplanet Science Congress 2024, Sep 2024, Berlin, Germany. pp.EPSC2024-177, ⟨10.5194/epsc2024-177⟩ |
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Design of the VenSpec-U instrument: a double UV imaging spectrometer to analyze sulfured gases in the Venus’ atmosphereInfrared Remote Sensing and Instrumentation XXXII. Proceedings SPIE 13144, Aug 2024, San Diego, United States. 33 p., ⟨10.1117/12.3028252⟩ |
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Ground-based thermal mapping of Venus: HDO and SO2 monitoring and upper limits of NH3, PH3 and HCN at the cloud topEGU General Assembly 2024, Apr 2024, Vienna and Online, Austria. pp.EGU24-4022, ⟨10.5194/egusphere-egu24-4022⟩ |
Sensitivity studies for the VeSUV/VenSpec-U instrument onboard ESA’s EnVision missionEGU General Assembly 2024, Apr 2024, Vienna and Online, Austria. pp.EGU24-16442, ⟨10.5194/egusphere-egu24-16442⟩ |
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Distribution and Variation of the Venusian Cloud-top Sulfur Dioxide Derived from Akatsuki UV ImagesEuroplanet Science Congress 2024, Sep 2024, Berlin, Germany. pp.EPSC2024-680, ⟨10.5194/epsc2024-680⟩ |
Design of the VenSpec-H instrument on ESA’s EnVision mission: development of critical elements, highlighting the FFCP, and gratingInfrared Remote Sensing and Instrumentation XXXII. Proceedings SPIE 13144, Aug 2024, San Diego, United States. 15 p., ⟨10.1117/12.3027637⟩ |
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Proton irradiation qualification of the vSWIR InGaAs imaging sensor for the VEM and VenSpec-M instruments on VERITAS and EnVisionInfrared Remote Sensing and Instrumentation XXXII. Proceedings SPIE 13144, Aug 2024, San Diego, United States. 13 p., ⟨10.1117/12.3028057⟩ |
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Observability of atmospheric spatial variability by the VeSUV/VenSpec-U instrument onboard ESA’s EnVision missionEuroplanet Science Congress 2024, Sep 2024, Berlin, Germany. pp.EPSC2024-465, ⟨10.5194/epsc2024-465⟩ |
Perspectives of infrared and ultraviolet spectroscopy in the exploration of the Venusian atmosphere and surface against the background of future missions: an overview and outlookInfrared Remote Sensing and Instrumentation XXXII. Ptroceedings SPIE 13144, spie, Aug 2024, San Diego, United States. 7 p., ⟨10.1117/12.3027282⟩ |
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Spectral mixing analysis of laboratory emissivity spectra for improved VenSpec-M/VEM data interpretationInfrared Remote Sensing and Instrumentation XXXII. Proceedings SPIE 13144, spie, Aug 2024, San Diego, United States. 16 p., ⟨10.1117/12.3027471⟩ |
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The Venus Emissivity Mapper (VEM): instrument design and development for VERITAS and EnVisionInfrared Remote Sensing and Instrumentation XXXII. Proceedings SPIE Volume 13144, SPIE, Aug 2024, San Diego, United States. 8 p., ⟨10.1117/12.3028082⟩ |
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Minor Species in Venus' Night Side Troposphere as Observed by VIRTIS-H/Venus ExpressVenus as a System, Nov 2023, Albuquerque, United States. pp.LPI Contribution No. 2891, id. 8003 |
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Spectroscopic Measurements of Sulfur Dioxide Above and Below Venus' Clouds: Past and FutureVenus Surface and Atmosphere 2023, Jan 2023, Houston, United States. pp.LPI Contribution No. 2807, id.8061 |
The VenSpec suite on the ESA Envision mission -a holistic investigation of the coupled surface atmosphere system of Venus55th Annual Meeting of the Division for Planetary Sciences, Oct 2023, San Antonio, United States. pp.id. 507.03 |
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Characterisation of the sensitivity to bias using a gain matrix formulation for the VeSUV/VenSpec-U instrument onboard ESA’s EnVision missionEGU General Assembly 2023, Apr 2023, Vienna (Austria), Austria. pp.EGU23-8312, ⟨10.5194/egusphere-egu23-8312⟩ |
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Scientific interest for a UV spectrometer to study Uranus and its satellitesUranus Flagship: Investigations and Instruments for Cross-Discipline Science Workshop, Jul 2023, Pasadena, United States. pp.LPI Contribution No. 2808, 2023, id. 8052 |
Science objective and status of the EnVision Mission to Venus55th Annual Meeting of the Division for Planetary Sciences, Oct 2023, San Antonio, United States. pp.id. 507.05, ⟨10.5194/egusphere-egu24-18247⟩ |
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EnVision: Understanding Why Earth's Closest Neighbor Is So Different54th Lunar and Planetary Science Conference, Mar 2023, The Woodlands, United States. pp.LPI Contribution No. 2806, id.1764, ⟨10.5194/epsc2021-414⟩ |
EnVision: a Nominal Science Phase Spanning Six Venus Sidereal DaysEGU General Assembly 2023, Apr 2023, Vienna (Austria), Austria. pp.EGU23-9889, ⟨10.5194/egusphere-egu23-9889⟩ |
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Atmospheric Chemistry on Venus: Current Understanding, Open Questions, and Upcoming MissionsVenus Surface and Atmosphere, Jan 2023, Houston, United States. pp.LPI Contribution No. 2807, id.8073 |
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The VenSpec suite on the ESA Envision mission -a holistic investigation of the coupled surface atmosphere system of VenusEuroplanet Science Congress 2022, Sep 2022, Granada, Spain. pp.EPSC2022-374 |
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Constraints on the existence of low-mass planets with supercritical hydrospheresEuroplanet Science Congress 2022, Sep 2022, Granada, Spain. pp.EPSC2022-418 |
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The Envision Mission to VenusEGU General Assembly 2022, May 2022, Vienna, Austria. pp.EGU22-8391, ⟨10.5194/egusphere-egu22-8391⟩ |
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The Envision Mission to Venus53rd Lunar and Planetary Science Conference, Mar 2022, The Woodlands, United States. pp.LPI Contribution No. 2678, 2022, id.2948 |
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Turbulent vertical mixing in the Venus cloud layer20th Meeting of the Venus Exploration and Analysis Group (VEXAG), Nov 2022, Albuquerque, United States. pp.LPI Contribution No. 2688 |
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The Venus surface emissivity mapper on the NASA VERITAS mission and the VenSpec suite on the ESA EnVision mission53rd Lunar and Planetary Science Conference, Mar 2022, The Woodlands, United States. pp.LPI Contribution No. 2678, 2022, id.2071 |
Day-Night Cloud Asymmetry Inhibits Early Ocean Formation on Venus and Telluric PlanetsAncient Venus Conference 2022, Jul 2022, Online, Unknown Region. pp.LPI Contribution No. 2680, id.2009 |
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EnVision: a Nominal Science Phase Spanning Six Venus Sidereal Days (Four Earth Years)AGU Fall Meeting 2022, Dec 2022, Chicago, United States. pp.id. P55B-05 |
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EnVision: understanding why our closest neighbour is so differentEuroplanet Science Congress 2022, Sep 2022, Granada, Spain. pp.EPSC2022-1097 |
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Minor species measurements below the clouds of Venus using VIRTIS-H/Venus Express data set.Europlanet Science Congress 2022, Sep 2022, Granada, Spain. pp.EPSC2022-7, ⟨10.5194/epsc2022-7⟩ |
Population study: Exploring the transition from Super-Earth to Sub-Neptune with a Hubble transmission survey44th COSPAR Scientific Assembly, Jul 2022, Athens, Greece. pp.Abstract B6.1-0014-22 |
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Escape of moderately volatile elements from protoplanets and its potential effect on habitabilityEuroplanet Science Congress 2022, Sep 2022, Granada, Spain. pp.EPSC2022-999, ⟨10.5194/epsc2022-999⟩ |
Long-term Plan to Monitor Venus using Earth-orbiting CubeSats: Chasing the Long-term Variability of Our Nearest Neighbor Planet Venus (CLOVE)44th COSPAR Scientific Assembly, Jul 2022, Online, Unknown Region. pp.Abstract B4.1-0032-22 |
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Interior structure and possible existence of irradiated ocean planets16th Europlanet Science Congress 2022, Sep 2022, Granada, Spain. pp.EPSC2022-904, ⟨10.5194/epsc2022-904⟩ |
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Consolidating the radiative transfer code to analyze VenSpec-H measurementsEuroplanet Science Congress 2022, Sep 2022, Granada, Spain. ⟨10.5194/epsc2022-899⟩ |
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VenSpec-H: Introduction to Instrument and ConsortiumEuroplanet Science Congress 2022, Sep 2022, Granada, Spain. pp.EPSC2022-1113, ⟨10.5194/epsc2022-1113⟩ |
Venus' atmosphere: an overview before next exploration missions44th COSPAR Scientific Assembly, Jul 2022, Athens, Greece. pp.Abstract C3.1-0002-22 |
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The VenSpec-H instrument onboard EnVisionAGU Fall Meeting 2022, Dec 2022, Chicago, United States. pp.id. P51B-12 |
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HST WFC3 G141 data analysis: exploring the transition from Super-Earth to Sub-NeptuneEuropean Planetary Science Congress. EPSC 2021, Sep 2021, Virtual Meeting, France. ⟨10.5194/epsc2021-194⟩ |
Characterising the atmospheres of the two warm Neptune-like planets HD 106315 c and HD 3167 c with the HST/WFC3 Camera43rd COSPAR Scientific Assembly, Jan 2021, Sydney, Australia. pp.Abstract B6.1-0002-21 (oral), id.498 |
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Day-Night Cloud Asymmetry Inhibits Early Ocean Formation on VenusVenera-D: Venus Cloud Habitability System Workshop, Nov 2021, Virtual Meeting, Unknown Region. pp.LPI Contribution No. 2629, id.4051 |
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Characterisation of the interior structures and atmospheres of multiplanetary systemsPlato Mission Conference 2021, Oct 2021, Virtual, Spain. ⟨10.5281/zenodo.5564164⟩ |
Characterizing the atmospheres of the two warm Neptune-liked planets HD 106315 c and HD 3167 c with the HST/WFC3 CameraAmerican Astronomical Society meeting #237, Jan 2021, Virtual Meeting, Unknown Region. pp.id. 437.02 |
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Detecting Venus' volcanic gas plumes with VenSpec-HEuropean Planetary Science Congress 2021, Sep 2021, Online, United States. pp.EPSC2021-678, ⟨10.5194/epsc2021-678⟩ |
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Characterising the interior structures and atmospheres of multiplanetary systems.European Planetary Science Congress. EPSC 2021, Sep 2021, Virtual Meeting, France. pp.306-322, ⟨10.5194/epsc2021-44⟩ |
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Mass-Radius relationships of small, highly irradiated exoplanets with small water mass fractionsEuropean Planetary Science Congress. EPSC 2021, Sep 2021, Virtual Meeting, France. ⟨10.5194/epsc2021-249⟩ |
Observability of temperate exoplanets with Ariel53rd AAS Division of Planetary Science meeting, Oct 2021, Virtual, United States. pp.id.212.13 |
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Turbulent vertical mixing of H2O and SO2 in the Venus cloud layerEuropean Planetary Science Congress 2021, Sep 2021, Online, Unknown Region. pp.EPSC2021-631, ⟨10.5194/epsc2021-631⟩ |
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Io's dry body shaped by atmospheric instabilityEuropean Planetary Science Congress. EPSC 2021, Sep 2021, Virtual Meeting, France. pp.306-322, ⟨10.5194/epsc2021-187⟩ |
Need for Updates to the Venus International Reference Model (VIRA)43rd COSPAR Scientific Assembly 2021, Jan 2021, sydney, Australia. pp.Abstract B4.4-0009-21 (oral), id.428 |
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VenSpec-H: an Infrared Spectrometer to Study Venus' ActivityAGU Fall Meeting 2021, Dec 2021, New Orleans, United States. pp.id. P35H-2225 |
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Characterising the interior structures and atmospheres of Multiplanetary systemsSF2A-2021: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, Jun 2021, On Line, France. pp.355-358 |
Venus exploration in the Horizon 2061: the pertinence of a sample return mission43rd COSPAR Scientific Assembly., Jan 2021, Sydney, Australia. pp.Abstract B0.7-0013-21 (oral), id.250 |
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Modeling the structure of irradiated ocean planets - implications for mass-radius relationshipsEuropean Planetary Science Congress. EPSC 2021, Sep 2021, Virtual Meeting, France. ⟨10.5194/epsc2021-27⟩ |
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The Venus Emissivity Mapper – Obtaining Global Mineralogy of Venus from Orbit on the ESA EnVision and NASA VERITAS missions to Venus.14th Europlanet Science Congress 2020, Sep 2020, Online, Unknown Region. pp.EPSC2020-260, ⟨10.5194/epsc2020-260⟩ |
Atmospheric Chemistry on Present-Day Venus and Earth: Unresolved Issues and Implications for Extrasolar PlanetsExoplanets in Our Backyard: Solar System and Exoplanet Synergies on Planetary Formation, Evolution, and Habitability, Feb 2020, Houston, United States. pp.LPI Contribution No. 2195 |
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A Stringent Upper Limit of the PH3 Abundance at the Cloud Top of VenusAGU Fall Meeting 2020, Dec 2020, Online, United States. pp.P092-05 |
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EnVision: Undestanding why Earth’s closest neighbour is so different18th Meeting of the Venus Exploration Analysis Group (VEXAG),, Nov 2020, Online, Unknown Region. pp.LPI Contribution No. 2356, id.8028 |
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The science goals of the EnVision Venus orbiter missionEuroplanet Science Congress 2020, Sep 2020, Online, Unknown Region. pp.EPSC2020-599, ⟨10.5194/epsc2020-599⟩ |
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A self-consistent thermodynamic approach to compute the interiors of irradiated ocean planetsEuroplanet Science Congress 2020, Sep 2020, Online, Unknown Region. pp.EPSC2020-610, ⟨10.5194/epsc2020-610⟩ |
Monitoring Venus cloud top: the VenSpec-U spectrometer on board ESA EnVisionEuroplanet Science Congress 2020, Sep 2020, Virtual Meeting, Germany. pp.EPSC2020-622 |
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Atmospheric noble gas isotope and bulk K/U ratios as a constraint on the origin and early evolution of Venus and EarthThe Main Belt: A Gateway to the Formation and Early Evolution of the Solar System, Jun 2019, Villasimius, Sardinia, Italy |
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The VenSpec suite on the ESA EnVision mission to Venus21st EGU General Assembly, EGU2019, Apr 2019, Vienna, Austria. pp.id.8665 |
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Ultraviolet albedo of Venus' clouds due to SPICAV and VIRTIS joint nadir observations onboard Venus ExpressEPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-1597-1 |
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The VenSpec suite on the ESA EnVision mission to VenusProceedings Volume 11128, Infrared Remote Sensing and Instrumentation XXVII, Aug 2019, San Diego, United States. pp.art. 1112804, ⟨10.1117/12.2529248⟩ |
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VenSpec-H, infrared spectrometer onboard EnVision to study Venus' volcanismEPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-1670-1 |
HDO and SO2 thermal mapping on Venus : Statistical analysis of the SO2 plumes21st EGU General Assembly, EGU2019, Apr 2019, Vienna (Austria), Austria. pp.id.4332 |
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Intense decadal variations of Venus' UV albedo, and its impact on solar heating rate and atmospheric dynamicsEPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-66-1 |
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Preparing EnVision: SO<sub>2</sub> measurements below and above Venus' cloudsEPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-253-1 |
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Atmospheric Chemistry on Venus: An Overview of Unresolved Issues50th Lunar and Planetary Science Conference, Mar 2019, The Woodlands, United States. pp.LPI Contribution No. 2132, id.2374 |
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EnVision M5 Venus orbiter proposalEPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-1611-2 |
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Impact of Topography on Venus' Cloud Top Properties as Observed by HST50th Lunar and Planetary Science Conference, Mar 2019, The Woodlands, United States. pp.LPI Contribution No. 2132, id.2728 |
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Atmospheric noble gas isotope and bulk K/U ratios as a constraint on the early evolution of Venus and EarthEPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-1550-1 |
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Hyperspectral Observer for Venus Reconnaissance (HOVER) Larry W. Esposito, and the HOVER TeamEPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-340 |
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Spectroscopy of the Surface of Venus -in the Laboratory and from OrbitEPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-1358-1 |
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The Venus Emissivity Mapper -Obtaining Global Mineralogy of Venus from Orbit on the ESA EnVision and NASA VERITAS missions to Venus50th Lunar and Planetary Science Conference, Mar 2019, The Woodlands, United States. pp.LPI Contribution No. 2132, id.2046 |
EnVision: Understanding Why our most Earth-like Neighbour is so Different21st EGU General Assembly, EGU2019, Apr 2019, Vienna, Austria. pp.id.17377 |
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Intense decadal variation of Venus' 365-nm albedo and its impacts on the atmosphereInternational Venus Conference, May 2019, Niseko, Hokkaido, Japan |
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Ground-based mapping of SO<sub>2</sub> and HDO on Venus in the thermal infraredEPSC-DPS joint meeting, Sep 2019, Genève, Switzerland. pp.EPSC-DPS2019-83 |
Science objectives of the VenSpec-U channel on board EnVision21st EGU General Assembly, EGU2019, Apr 2019, Vienna, Austria. pp.id.4237 |
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Escape and fractionation of elements from planetary embryosEPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-1345 |
VenSpec-H, infrared spectrometer onboard EnVision to study Venus' volcanism21st EGU General Assembly, EGU2019, Apr 2019, Vienna, Austria. pp.id.17644 |
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High-Level Science Products of SPICAM (Mars Express) and SPICAV (Venus Express)EPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland, Switzerland. pp.EPSC-DPS2019-579-1 |
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Venus Surface Oxidation and Weatehring as Viewed from Orbit with Six-Window VNIR Spectroscopy16th Meeting of the Venus Exploration and Analysis Group (VEXAG), Nov 2018, Laurel, Maryland, United States. pp.LPI Contribution No. 2137, id.8015 |
Spectral albedo of Venus clouds in the UV as measured onboard the VEX orbiter42nd COSPAR Scientific Assembly, Jul 2018, Pasadena, United States. pp.Abstract id. C3.1-2-18 |
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The Venus Emissivity Mapper (VEM): Obtaining global mineralogy of Venus from orbitInfrared Remote Sensing and Instrumentation XXVI, Aug 2018, San Diego, United States. pp.art. 107650D, ⟨10.1117/12.2320112⟩ |
HDO and SO2 thermal mapping on Venus: Statistical analysis of the SO2 plumes and comparison with space dataEGU General Assembly Conference Abstracts, Apr 2018, Vienna, Austria. pp.1865 |
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14 years of Mars’ atmosphere monitoring by SPICAM on Mars ExpressScientific Workshop: “From Mars Express to ExoMars”, Feb 2018, Madrid, Spain. 2 p |
Venus cloud top as observed by SPICAV-UV/Venus Express: SO2 , O3 and clouds20th EGU General Assembly, Apr 2018, Vienna, Austria. pp.6270 |
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Early Evolution of Super-Earths: From Magma Ocean to Temperate Surface ConditionsAmerican Geophysical Union, Fall Meeting 2018, Dec 2018, Washington, United States. pp.abstract #P42A-07 |
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Progress towards a post-Venus Express Clouds & Haze reference model for Venus42nd COSPAR Scientific Assembly, Jul 2018, Pasadena, United States |
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Early evolution of Venus and Earth constrained by the reproduction of measured Ar, Ne isotope and K/U elemental ratiosEuropean Planetary Science Congress 2018, Sep 2018, Berlin, Germany. pp.EPSC2018-291 |
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The Venus Emissivity Mapper (VEM) — Obtaining Global Mineralogy of Venus from Orbit16th Meeting of the Venus Exploration and Analysis Group (VEXAG), Nov 2018, Laurel, Maryland, United States. pp.LPI Contribution No. 2137, id.8023 |
Hubble's Role in Studies of Venus' Clouds, Climate and HabitabilityAmerican Astronomical Society, AAS Meeting #232, Jun 2018, Denver, United States. pp.id. 405.06 |
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Leveraging Rock Type, Mineralogy, and Oxidation State from Six-Window Emissivity Spectra at 440CEPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-1822 |
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Insights on Venus’Cloud Top Chemistry, Convective Activity and Topographyfrom HSTEPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-672-2 |
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Escape and fractionation of elements from planetary embryosEuropean Planetary Science Congress 2018, Sep 2018, Berlin, Germany. pp.EPSC2018-305 |
Understanding Venus: An International Effort42nd COSPAR Scientific Assembly, Jul 2018, Pasadena, United States. pp.Abstract id. PEX.1-16-18 |
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The Venus Emissivity Mapper conceptProceeding SPIE 10403, Infrared Remote Sensing and Instrumentation XXV, Aug 2017, San Diego, United States. ⟨10.1117/12.2275666⟩ |
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Reanalysis of the SPICAV-UV nadir spectra on the day side of Venus: SO<sub>2</sub> , O<sub>3</sub> and other UV absorbersEuropean Planetary Science Congress 2017, Sep 2017, Riga, Latvia. pp.PSC2017-165 |
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Mapping Venus Mineralogy and Chemistry In Situ from Orbit with Six-Window VNIR Spectroscopy15th Meeting of the Venus Exploration Analysis Group ( VEXAG ), Nov 2017, Laurel, Maryland, United States. LPI Contribution No. 2061, p.8004 |
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Distribution of SO<sub>2</sub> content at the night side of Venus' upper mesosphereInternational Venus Conference 2016, Apr 2016, Oxford, United Kingdom |
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Influence of Venus topography on the zonal wind and albedo at cloud top level : The role of stationary gravity wavesInternational Venus Conference 2016, Apr 2016, Oxford, United Kingdom |
A 1D radiative-convective model of H2O-CO2 atmospheres around young telluric planets: an updateEuropean Geosciences Union General Assembly 2016, Apr 2016, Vienna, Austria. pp.EGU2016-7316-1 |
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Advancing Venus Atmospheric Modeling via Coordinated HST-Akatsuki Observations47th Lunar and Planetary Science Conference, Mar 2016, The Woodlands, Texas, United States |
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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 |
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The Venus Emissivity Mapper (VEM) Concept47th Lunar and Planetary Science Conference, Mar 2016, The Woodlands, Texas, United States |
Observed correlation of Venus topography with the zonal wind and albedo at cloud top level: the role of stationary gravity waves.European Geosciences Union General Assembly 2016, Apr 2016, Vienna, Austria. pp.EGU2016-16126 |
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Venus : Observe it while it's hot !International Venus Conference 2016, Apr 2016, Oxford, United Kingdom |
The Venus Emissivity Mapper (VEM) conceptInfrared Remote Sensing and Instrumentation XXIV. Proceedings SPIE, Aug 2016, San Diego, United States. Paper 9973-26 |
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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 |
High-spectral resolution mid-UV spectrograph for Venus observingVenus : Science priorities for Laboratory Measurements and Instrument Definition Workshop, Apr 2015, Hampton, United States. pp.4024 |
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Sciences for Exoplanets and Planetary Systems : web sites and E-learningEuropean Planetary Science Congress 2015, Sep 2015, Nantes, France. pp.EPSC2015-748-6 |
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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Geographic distribution of zonal wind and UV albedo at cloud top level from VMC camera on Venus Express: Influence of Venus topography through stationary gravity waves vertical propagationEuropean Planetary Science Congress 2015, Sep 2015, Nantes, France. pp.EPSC2015-87 |
SPICAM on Mars Express: a 10 year in-depth survey of the Martian atmosphereEGU General Assembly 2015, Apr 2015, Vienna, Austria. pp.EGU2015-6376 |
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Study of Venus cloud layers with polarimetric data from SPICAV/VExEGU General Assembly 2014, Apr 2014, Vienna, Austria |
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Evidence for an orographic forcing of SO 2 observed above the clouds with SPICAV/Venus ExpressEuropean Planetary Science Congress 2014, Sep 2014, Cascais, Portugal. pp.EPSC2014-325 |
Magma ocean formation and outgassing, steam atmospheresISSI-BJ/ISSI Workshop, Aug 2014, Pékin, China |
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Measurements of carbon monoxide above Venus' cloud top from IRTF/CSHELL observationsEGU General Assembly 2014, Apr 2014, Vienna, Austria. pp.id.6599 |
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Composition and Chemistry of the Neutral Atmosphere of VenusEuropean Planetary Science Congress, Sep 2014, Cascais, Portugal. pp.EPSC2014-153 |
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Thermal structure of Venus' nightside upper atmosphere measured by SPICAV UV on Venus ExpressEuropean Planetary Science Congress 2014, Sep 2014, Cascais, Portugal. pp.EPSC2014-408 |
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SO2 measurements at Venus' cloud top: from Pioneer Venus Orbiter to Venus Express39th COSPAR Scientific Assembly, Jul 2012, Mysore, India |
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SO2 monitoring above Venus' clouds using VEx/SPICAV-UV nadir observationsEGU General Assembly 2012, Apr 2012, Vienna, Austria |
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Discovery and characterization of an ozone layer in Venus' atmosphereEuropean Geophysical Union General Assembly 2011, Apr 2011, Vienna, Austria |
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Looking for SO2: a spectroscopic study of Martian UV albedo using SPICAMFourth International Workshop on the Mars Atmosphere: Modelling and Observations, Feb 2011, Paris, France. 2 p |
Long-term monitoring SO<sub>2</sub> above the clouds of Venus using SPICAV-UV in nadir modeEuropean Geophysical Union General Assembly 2011, Apr 2011, Vienna, Austria. pp.EGU2011-2603 |
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Ozone on Mars and VenusEPSC-DPS Joint Meeting 2011, Oct 2011, Nantes, France |
Sulfur mono- and dioxides above Venus' clouds from SPICAV/SOIR solar occultationsEuropean Geophysical Union General Assembly 2011, Apr 2011, Vienna, Austria |
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Variability of SO2 at Venus' cloud top during the July 2009 brightening event as seen by SPICAV-UVEPSC-DPS Joint Meeting 2011, Oct 2011, Nantes, France |
Variability of SO2 above the clouds of Venus using Venus Express/SPICAV-UV in nadir modeEGU General Assembly 2010, May 2010, Vienna, Austria |
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Constraining SO2 in the atmospheres of Venus and Mars using SPICAV-UV & SPICAM-UV in nadir modeEuropean Planetary Science Congress 2010, Sep 2010, Rome, Italy |
SO2 above The clouds of Venus as measured by SPICAV-UV In Nadir42nd Annual Meeting of the Division for Planetary Sciences (DPS), Oct 2010, Pasadena, United States |
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Super Venus" : a 1D radiative-convective model of primitive Earth atmosphereInternational Venus Conference, Jun 2010, Aussois, France |
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Overview of SPICAV occultation results for the UV channel38th COSPAR Scientific Assembly, Jul 2010, Bremen, Germany |
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Sulfur dioxide above Venus' clouds: sounding by orbital solar occultations in UV and IR rangesEGU General Assembly 2010, May 2010, Vienna, Austria |
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Three Martian years of observations with SPICAM on Mars ExpressAmerican Geophysical Union, Fall Meeting 2010, Dec 2010, San Francisco, United States |
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Transport-driven formation of an ozone layer on Venus and Mars as evidenced by SPICAM and SPICAV42nd Annual Meeting of the Division for Planetary Sciences (DPS), Oct 2010, Pasadena, United States |
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An overview of SPICAV/SOIR results on the atmosphere of Venus from Venus Express Mission41st Annual Meeting of the Division for Planetary Sciences (DPS), Oct 2009, Puerto Rico, United States |
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Detection of SO<sub>2</sub> above the clouds of Venus using SPICAV/Venus ExpressEGU General Assembly 2009, Apr 2009, Vienna, Austria |
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Discovery of an Ozone Layer on Venus by SPICAV on Venus Express41st Annual Meeting of the Division for Planetary Sciences (DPS), Oct 2009, Puerto Rico, United States |
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Latitudinal Variations of SO2 Above the Clouds of Venus Using SPICAV-UV/Venus Express41st Annual Meeting of the Division for Planetary Sciences (DPS), Oct 2009, Puerto Rico, United States |
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Composition of the Venusian atmosphere after Venus ExpressEPSC (European Planetary Science Congress) 2009, Sep 2009, Potsdam, Germany |
Distribution of Carbon Monoxide and Other Minor Species In The Lower Atmosphere of Venus Using Venus Express/VIRTIS-M-IR DataAmerican Astronomical Society, DPS meeting #39, 2007, Orlando (Florida), United States. pp.502 |
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Distribution Of Carbon Monoxide And Other Minor Species In The Lower Atmosphere Of Venus Using Venus Express/VIRTIS-M-IR DataAAS/Division for Planetary Sciences Meeting #39, AAS, Oct 2007, Orlando, United States. pp.502 |
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3D Simulations of the Early Mars Climate with a General Circulation ModelThird International Conference on Mars Polar Science and Exploration, Oct 2003, Alberta, Canada. pp.8070 |
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The VenSpec-U Ultraviolet Spectral Imager on board EnVisionEuroplanet Science Congress 2024, Sep 2024, Berlin, Germany. EPSC Abstracts, 17, pp.EPSC2024-335, 2024, ⟨10.5194/epsc2024-335⟩ |
Irradiation qualification campaign of the vSWIR InGaAs imaging sensor for the VEM and VenSpec-M instruments on VERITAS and EnVisionEuroplanet Science Congress 2024, Sep 2024, Berlin, Germany. EPSC Abstracts, 17, pp.EPSC2024-1004, 2024, ⟨10.5194/epsc2024-1004⟩ |
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Assessing near-surface radiance levels based on VIRTIS spectra to prepare VenSpec-H scienceEuroplanet Science Congress 2024, Sep 2024, Berlin, Germany. EPSC Abstracts, 17, pp.EPSC2024-1025, 2024, ⟨10.5194/epsc2024-1025⟩ |
Future Exploration of Venus: International Coordination and Collaborations43rd COSPAR Scientific Assembly 2021, Jan 2021, Sydney, Australia. 43, Abstract B4.4-0028-21, id p.445., 2021 |
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Characterising the interior structures and atmospheres of transiting super-Earths and sub-NeptunesTESS Science Conference II (TSC2), Aug 2021, On Line, United States. pp.id.47, ⟨10.5281/zenodo.5123312⟩ |
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The Venus Emissivity Mapper — Investigating the Atmospheric Structure and Dynamics of Venus' Polar Region49th Lunar and Planetary Science Conference, Mar 2018, The Woodlands, United States. pp.LPI Contribution No. 2083, id.2386 |
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Venus Emissivity Mapper – Investigating the Atmospheric Structure and Dynamics of Venus' Polar Region15th Meeting of the Venus Exploration and Analysis Group (VEXAG), Nov 2017, Laurel, Maryland, United States. pp.LPI Contribution No. 2061, 2017 |
Sulfur Dioxide variability in the Venus atmosphere26th IUGG, General Assembly 2015, Jun 2015, Prague, France |
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Study of Venus cloud layers by polarimetry using SPICAV/VExEGU General Assembly 2015, Apr 2015, Vienna, Austria. pp.EGU2015-1656 |
Geographic distribution of zonal wind and UV albedo at cloud top level from VMC camera on Venus Express: Influence of Venus topography through stationary gravity waves vertical propagation.EGU General Assembly 2015, Apr 2015, Vienna, Austria. pp.EGU2015-14228, 2015 |
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Sulfur Dioxide variability in the Venus AtmosphereEuropean Planetary Science Congress 2015, Sep 2015, Nantes, France. 10, pp.EPSC2015-122 |
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Influence of initial CO2 content on a planet surface conditions at the end of the magma ocean phaseEuropean Planetary Science Congress 2015, Sep 2015, Nantes, France. European Planetary Science Congress 2015, 10, pp.EPSC2015-823, 2015 |
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Study of Venus cloud layers by polarimetry using SPICAV/VExAstronomical Polarimetry 2014, May 2014, Grenoble, France. , 2014 |
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Possible Influence of Venus Topography on the Zonal Wind and UV albedo at Cloud Top LevelAGU Fall Meeting 2014, Dec 2014, San Francisco, United States. pp.P21B-3916, 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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Cooling of an early Earth magma ocean in interaction with the atmosphereEPSC-DPS Joint Meeting 2011, Oct 2011, Nantes, France. pp.EPSC-DPS2011-798-1 |
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Sulphur oxides in Venus mesosphere detected from SPICAV/SOIR VEX solar occultationEPSC-DPS Joint Meeting 2011, Oct 2011, Nantes, France |
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An atmospheric model designed for integration into coupled models of magma ocean planetsEPSC-DPS Joint Meeting 2011, Oct 2011, Nantes, France |
Rayleigh ScatteringMuriel Gargaud, William M. Irvine, Ricardo Amils, Philippe Claeys, Henderson James Cleaves, Maryvonne Gerin, Daniel Rouan, Tilman Spohn, Stéphane Tirard, Michel Viso (eds). Encyclopedia of Astrobiology, Springer Berlin Heidelberg, pp.2629-2631, 2023, Print ISBN: 978-3-662-65092-9 / Online ISBN: 978-3-662-65093-6. ⟨10.1007/978-3-662-65093-6_5493⟩ |
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Radiative Transfer (Atmospheres)Muriel Gargaud, William M. Irvine, Ricardo Amils, Philippe Claeys, Henderson James Cleaves, Maryvonne Gerin, Daniel Rouan, Tilman Spohn, Stéphane Tirard, Michel Viso (eds). Encyclopedia of Astrobiology, Springer Berlin Heidelberg, pp.2585-2595, 2023, Print ISBN: 978-3-662-65092-9 / Online ISBN: 978-3-662-65093-6. ⟨10.1007/978-3-662-65093-6_5486⟩ |
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Mie ScatteringMuriel Gargaud, William M. Irvine, Ricardo Amils, Philippe Claeys, Henderson James Cleaves, Maryvonne Gerin, Daniel Rouan, Tilman Spohn, Stéphane Tirard, Michel Viso (eds). Encyclopedia of Astrobiology, Springer Berlin Heidelberg, pp.1948-1952, 2023, Print ISBN: 978-3-662-65092-9 / Online ISBN: 978-3-662-65093-6. ⟨10.1007/978-3-662-65093-6_5492⟩ |
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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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Prélude à la mission Venus Express : étude de l'atmosphère par spectro-imagerie infrarougeAstrophysique [astro-ph]. Université Paris-Diderot - Paris VII, 2006. Français. ⟨NNT : ⟩ |