activity
20232026
most citedA 3D picture of moist-convection inhibition in hydrogen-rich atmospheres: Implications for K2-18 b

41 citations · 78 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2026

Latitudinal variations in Neptune's temperature profile observed with ALMA

Óscar Carrión-González, Raphael Moreno, Emmanuel Lellouch +5

Despite the low solar irradiation it receives, Neptune shows a very active atmosphere with some of the most intense dynamics observed in Solar System atmospheres. Characterizing th…

astro-ph.EP2024★ 5 cited

Ionospheric conductances at the giant planets of the Solar System:a comparative study of ionization sources and the impact of meteoric ions

Noé Clément, Yuki Nakamura, Michel Blanc +2

The dynamics of giant planet magnetospheres is controlled by a complex interplay between their fast rotation, their interaction with the solar wind, and their diverse internal plas…

astro-ph.EP2024★ 6 cited

Storms and convection on Uranus and Neptune: impact of methane abundance revealed by a 3D cloud-resolving model

Noé Clément, Jérémy Leconte, Aymeric Spiga +8

Uranus and Neptune have atmospheres dominated by molecular hydrogen and helium. In the upper troposphere, methane is the third main molecule and condenses, yielding a vertical grad…

astro-ph.EP2024

The radiative and dynamical impact of clouds in the atmosphere of the hot Jupiter WASP-43 b

Lucas Teinturier, Benjamin Charnay, Aymeric Spiga +6

Hot Jupiters exhibit large day-night temperature contrasts. Their cooler nightsides are thought to host clouds. However, the exact nature of these clouds, their spatial distributio…

astro-ph.EP2024★ 41 cited

A 3D picture of moist-convection inhibition in hydrogen-rich atmospheres: Implications for K2-18 b

Jérémy Leconte, Aymeric Spiga, Noé Clément +9

While small, Neptune-like planets are among the most abundant exoplanets, our understanding of their atmospheric structure and dynamics remains sparse. In particular, many unknowns…

astro-ph.EP2023★ 16 cited

Source of radio emissions induced by the Galilean moons Io, Europa and Ganymede: in situ measurements by Juno

C. K. Louis, P. Louarn, B. Collet +13

At Jupiter, part of the auroral radio emissions are induced by the Galilean moons Io, Europa and Ganymede. Until now, except for Ganymede, they have been only remotely detected, us…

astro-ph.EP2023★ 10 cited

Doppler wind measurements in Neptune's stratosphere with ALMA

Óscar Carrión-González, Raphael Moreno, Emmanuel Lellouch +6

Neptune's tropospheric winds are among the most intense in the Solar System, but the dynamical mechanisms that produce them remain uncertain. Measuring wind speeds at different pre…