activity
20102025
most citedRevealing the Mysteries of Venus: The DAVINCI Mission

181 citations · 644 across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.EP2025★ 1 cited

Comparison of General Circulation Models of the Venus upper atmosphere

Antoine Martinez, Hiroki Karyu, Amanda Brecht +7

In the context of future Venusian missions, it is crucial to improve our understanding of Venus upper atmosphere through 3D modeling, notably for spacecraft orbit computation. This…

astro-ph.EP2025★ 1 cited

The effect of near-surface winds on surface temperature and dust transport on Venus

Maxence Lefèvre, Sébastien Lebonnois, Aymeric Spiga +1

The knowledge of the Venus near-surface atmosphere is sparse. Few spacecrafts landed on the surface and measured winds with amplitudes below 1 m/s. The diurnal cycle of the wind am…

astro-ph.EP2025★ 5 cited

Evaluation of new radio occultation observations among small satellites at Venus by data assimilation

Yukiko Fujisawa, Norihiko Sugimoto, Chi Ao +5

We conducted observing system simulation experiments (OSSEs) for radio occultation measurements (RO) among small satellites, which are expected to be useful for future Venus missio…

astro-ph.EP2024★ 62 cited

Latitudinal Variation of Clouds' Structure Responsible for Venus' Cold Collar

I. Garate-Lopez, Sébastien Lebonnois

Global Climate Models (GCM) are very useful tools to study theoretically the general dynamics and specific phenomena in planetary atmospheres. In the case of Venus, several GCMs su…

astro-ph.EP2024★ 13 cited

Validation of the IPSL Venus GCM Thermal Structure with Venus Express Data

Pietro Scarica, Itziar Garate-Lopez, Sebastien Lebonnois +4

General circulation models (GCMs) are valuable instruments to understand the most peculiar features in the atmospheres of planets and the mechanisms behind their dynamics. Venus ma…

astro-ph.EP2023★ 4 cited

3D Global climate model of an exo-Venus: a modern Venus-like atmosphere for the nearby super-Earth LP 890-9 c

Diogo Quirino, Gabriella Gilli, Lisa Kaltenegger +6

The recently discovered super-Earth LP 890-9 c is an intriguing target for atmospheric studies as it transits a nearby, low-activity late-type M-dwarf star at the inner edge of the…

astro-ph.EP2022★ 181 cited

Revealing the Mysteries of Venus: The DAVINCI Mission

James B. Garvin, Stephanie A. Getty, Giada N. Arney +36

The Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging (DAVINCI) mission described herein has been selected for flight to Venus as part of the NASA Discover…

astro-ph.EP2021★ 7 cited

Gravitational atmospheric tides as a probe of Titan's interior: Application to Dragonfly

Benjamin Charnay, Gabriel Tobie, Sébastien Lebonnois +1

Context: Saturn's massive gravity is expected to causes a tide in Titan's atmosphere, producing a surface pressure variation through the orbit of Titan and tidal winds in the tropo…

astro-ph.EP2021★ 5 cited

Characterising atmospheric gravity waves on the nightside lower clouds of Venus: a systematic analysis

J. E. Silva, P. Machado, J. Peralta +3

We present the detection and characterisation of mesoscale waves on the lower clouds of Venus using images from the Visible Infrared Thermal Imaging Spectrometer onboard the Europe…

astro-ph.IM2021★ 27 cited

Ariel: Enabling planetary science across light-years

Giovanna Tinetti, Paul Eccleston, Carole Haswell +313

Ariel, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, was adopted as the fourth medium-class mission in ESA's Cosmic Vision programme to be launched in 2029. Durin…

astro-ph.EP2021★ 36 cited

Venus upper atmosphere revealed by a GCM: II. Model validation with temperature and density measurements

Gabriella Gilli, Thomas Navarro, Sebastien Lebonnois +5

An improved high-resolution ground-to-thermosphere version of the Institut Pierre-Simon Laplace (IPSL) Venus General Circulation Model (VGCM), including non-orographic gravity wave…

astro-ph.EP2019★ 43 cited

Seasonal changes in the middle atmosphere of Titan from Cassini/CIRS observations: temperature and trace species abundance profiles from 2004 to 2017

Christophe Mathé, Sandrine Vinatier, Bruno Bézard +6

The Cassini/Composite InfraRed Spectrometer (CIRS) instrument has been observing the middle atmosphere of Titan over almost half a Saturnian year. We used the CIRS dataset processe…

astro-ph.EP2019★ 12 cited

The Physical Origin of the Venus Low Atmosphere Chemical Gradient

Daniel Cordier, David A. Bonhommeau, Sara Port +3

Venus shares many similarities with the Earth, but concomitantly, some of its features are extremely original. This is especially true for its atmosphere, where high pressures and…

astro-ph.EP2019★ 54 cited

Long-term variations of Venus' 365-nm albedo observed by Venus Express, Akatsuki, MESSENGER, and Hubble Space Telescope

Yeon Joo Lee, Kandis-Lea Jessup, Santiago Perez-Hoyos +16

An unknown absorber near the cloud top level of Venus generates a broad absorption feature from the ultraviolet (UV) to visible, peaking around 360 nm, and therefore plays a critic…

astro-ph.EP2019★ 22 cited

Seasonal evolution of temperatures in Titan's lower stratosphere

M. Sylvestre, N. A. Teanby, J. Vatant d'Ollone +4

The Cassini mission offered us the opportunity to monitor the seasonal evolution of Titan's atmosphere from 2004 to 2017, i.e. half a Titan year. The lower part of the stratosphere…

astro-ph.EP2019★ 39 cited

Mesoscale modeling of Venus' bow-shape waves

Maxence Lefèvre, Aymeric Spiga, Sébastien Lebonnois

The Akatsuki instrument LIR measured an unprecedented wave feature at the top of Venusian cloud layer. Stationary bow-shape waves of thousands of kilometers large lasting several E…

astro-ph.EP2018★ 56 cited

Global climate modeling of Saturn's atmosphere. Part II: multi-annual high-resolution dynamical simulations

Aymeric Spiga, Sandrine Guerlet, Ehouarn Millour +9

The Cassini mission unveiled the intense and diverse activity in Saturn's atmosphere: banded jets, waves, vortices, equatorial oscillations. To set the path towards a better unders…

astro-ph.EP2011★ 57 cited

Titan's lakes chemical composition: sources of uncertainties and variability

D. Cordier, O. Mousis, J. I. Lunine +5

Between 2004 and 2007 the instruments of the CASSINI spacecraft discovered hydrocarbon lakes in the polar regions of Titan. We have developed a lake-atmosphere equilibrium model al…

astro-ph.EP2010★ 19 cited

About the possible role of hydrocarbon lakes in the origin of Titan's noble gas atmospheric depletion

D. Cordier, O. Mousis, J. I. Lunine +4

An unexpected feature of Titan's atmosphere is the strong depletion in primordial noble gases revealed by the Gas Chromatograph Mass Spectrometer aboard the Huygens probe during it…