431 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of CambridgeGB5 papers
- University of OxfordGB5 papers
- University of ReadingGB5 papers
- Centre National de la Recherche ScientifiqueFR3 papers
- University of ExeterGB3 papers
- University of LeedsGB3 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR2 papers
- Czech Academy of SciencesCZ2 papers
- Deutscher WetterdienstDE2 papers
- European Centre for Medium-Range Weather ForecastsGB2 papers
- Imperial College LondonGB2 papers
- Met OfficeGB2 papers
5 papers · 1 filter
Structure, variability, and origin of the low-latitude nightglow continuum between 300 and 1,800 nm: Evidence for HO emission in the near-infrared
Stefan Noll, John M. C. Plane, Wuhu Feng +5
The Earth's mesopause region between about 75 and 105 km is characterised by chemiluminescent emission from various lines of different molecules and atoms. This emission was and is…
Lightning-induced chemistry on tidally-locked Earth-like exoplanets
Marrick Braam, Paul I. Palmer, Leen Decin +5
Determining the habitability and interpreting atmospheric spectra of exoplanets requires understanding their atmospheric physics and chemistry. We use a 3-D Coupled Climate-Chemist…
Implications of three-dimensional chemical transport in hot Jupiter atmospheres: results from a consistently coupled chemistry-radiation-hydrodynamics model
Benjamin Drummond, Eric Hebrard, Nathan J. Mayne +9
We present results from a set of simulations using a fully coupled three-dimensional (3D) chemistry-radiation-hydrodynamics model and investigate the effect of transport of chemica…
Ozone chemistry on tidally locked M dwarf planets
Jack S. Yates, Paul I. Palmer, James Manners +4
We use the Met Office Unified Model to explore the potential of a tidally locked M dwarf planet, nominally Proxima Centauri b irradiated by a quiescent version of its host star, to…
Identifiable Acetylene Features Predicted for Young Earth-like Exoplanets with Reducing Atmospheres undergoing Heavy Bombardment
P. B. Rimmer, M. Ferus, I. P. Waldmann +14
The chemical environments of young planets are assumed to be largely influenced by impacts of bodies lingering on unstable trajectories after the dissolution of the protoplanetary…