8 May 2020 | Atmospheric convection plays a key role in the climate of tidally-locked terrestrial exoplanets: insights from high-resolution simulations
| Sergeev, D; Lambert, F; Mayne, N; et al. |
28 August 2018 | Exonephology: Transmission spectra from a 3D simulated cloudy atmosphere of HD209458b (article)
| Lines, S; Manners, J; Mayne, NJ; et al. |
21 April 2020 | The first Met Office Unified Model-JULES Regional Atmosphere and Land configuration, RAL1
| Bush, M; Allen, T; Bain, C; et al. |
16 July 2021 | The impact of mixing treatments on cloud modelling in 3D simulations of hot Jupiters
| Christie, DA; Mayne, NJ; Lines, S; et al. |
16 July 2020 | Implications of different stellar spectra for the climate of tidally locked Earth-like exoplanets (article)
| Eager, J; Reichelt, D; Mayne, N; et al. |
26 February 2018 | The influence of a sub-stellar continent on the climate of a tidally-locked exoplanet
| Mayne, NJ; Lewis, N; Lambert, FH; et al. |
10 April 2020 | Influences of Local and Remote Conditions on Tropical Precipitation and Its Response to Climate Change
| Saint-Lu, M; Chadwick, R; Lambert, FH; et al. |
22 January 2019 | The Limits of the Primitive Equations of Dynamics for Warm, Slowly Rotating Small Neptunes and Super Earths (article)
| Mayne, NJ; Drummond, B; Debras, F; et al. |
12 December 2018 | The limits of the primitive equations of dynamics for warm, slowly rotating Small Neptunes and Super Earths (dataset)
| Mayne, NJ; Drummond, B; Debras, F; et al. |
11 April 2017 | The Met Office Unified Model Global Atmosphere 6.0/6.1 and JULES Global Land 6.0/6.1 configurations
| Walters, D; Boutle, I; Brooks, M; et al. |
14 May 2019 | The Met Office Unified Model Global Atmosphere 7.0/7.1 and JULES Global Land 7.0 configurations
| Walters, D; Baran, AJ; Boutle, I; et al. |
9 June 2020 | Mineral dust increases the habitability of terrestrial planets but confounds biomarker detection (article)
| Boutle, I; Joshi, M; Lambert, F; et al. |
16 April 2020 | Mineral dust increases the habitability of terrestrial planets but confounds biomarker detection (dataset)
| Boutle, I; Joshi, M; Lambert, F; et al. |
2024 | A mixed finite-element, finite-volume, semi-implicit discretisation for atmospheric dynamics: Spherical geometry
| Melvin, T; Shipway, B; Wood, N; et al. |
27 January 2023 | A modern-day Mars climate in the Met Office Unified Model: dry simulations
| McCulloch, D; Sergeev, D; Mayne, N; et al. |
15 March 2018 | Observable signatures of wind--driven chemistry with a fully consistent three dimensional radiative hydrodynamics model of HD 209458b
| Drummond, B; Mayne, NJ; Manners, J; et al. |
15 March 2018 | Observable signatures of wind-driven chemistry with a fully consistent three dimensional radiative hydrodynamics model of HD 209458b (article)
| Drummond, B; Mayne, NJ; Manners, J; et al. |
1 July 2019 | Overcast on Osiris: 3D radiative-hydrodynamical simulations of a cloudy hot Jupiter using the parametrized, phase-equilibrium cloud formation code EDDYSED (article)
| Lines, S; Mayne, N; Manners, J; et al. |
8 January 2020 | Ozone chemistry on tidally locked M dwarf planets
| Yates, J; Palmer, P; Manners, J; et al. |
28 May 2024 | Reduction in the Tropical High Cloud Fraction in Response to an Indirect Weakening of the Hadley Cell
| Natchiar, SRM; Webb, MJ; Lambert, FH; et al. |