activity
20022026
most citedImplications of three-dimensional chemical transport in hot Jupiter atmospheres: results from a consistently coupled chemistry-radiation-hydrodynamics model

95 citations · 610 across the 25 of their papers we have counts for

collaborators

24 papers

astro-ph.EP2026

Three-dimensional transport-induced chemistry on temperate sub-Neptune K2-18b, Part II: the combined effects of atmospheric dynamics and chemical reactions

Jiachen Liu, Duncan Christie, Jun Yang +1

The upper atmospheres of temperate sub-Neptunes are strongly influenced by atmospheric dynamics due to their cool equilibrium temperature and thereby longer chemical timescales tha…

astro-ph.EP2025

The Impact of Different Haze Types on the Atmosphere and Observations of Hot Jupiters: 3D Simulations of HD 189733b, HD209458b and WASP-39b

Mei Ting Mak, Denis Sergeev, Nathan Mayne +6

We present the results from the simulations of the atmospheres of hot-Jupiters HD189733b, HD209458b and WASP-39b, assuming the presence of three different types of haze. Using a 3D…

astro-ph.EP2025

Geometric Considerations in Hot Jupiter Magnetic Drag Models

Duncan A. Christie, Tom M. Evans-Soma, Nathan J. Mayne +1

Magnetic fields are expected to impact the atmospheric dynamics of hot and ultra-hot Jupiters due to their increased ionization fractions, compared to that of cooler exoplanets, bu…

astro-ph.EP2024★ 10 cited

3D simulations of TRAPPIST-1e with varying CO2, CH4 and haze profiles

Mei Ting Mak, Denis Sergeev, Nathan Mayne +6

Using a 3D General Circulation Model, the Unified Model, we present results from simulations of a tidally-locked TRAPPIST-1e with varying carbon dioxide CO2 and methane CH4 gas con…

astro-ph.EP2024★ 1 cited

Quenching-driven equatorial depletion and limb asymmetries in hot Jupiter atmospheres: WASP-96b example

Maria Zamyatina, Duncan A. Christie, Eric Hébrard +11

Transport-induced quenching in hot Jupiter atmospheres is a process that determines the boundary between the part of the atmosphere at chemical equilibrium and the part of the atmo…

astro-ph.EP2024

The impact of the explicit representation of convection on the climate of a tidally locked planet in global stretched-mesh simulations

Denis E. Sergeev, Ian A. Boutle, F. Hugo Lambert +5

Convective processes are crucial in shaping exoplanetary atmospheres but are computationally expensive to simulate directly. A novel technique of simulating moist convection on tid…