activity
20182026
most citedLatitudinal variation in the abundance of methane (CH4) above the clouds in Neptune's atmosphere from VLT/MUSE Narrow Field Mode Observations

44 citations · 122 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.IM2026

A research roadmap for assessing the feasibility of warming Mars

E. S. Kite, A. Essunfeld, M. H. Hecht +22

This roadmap outlines research pathways to determine whether Mars could be warmed with non-biological methods. It does not presuppose that warming Mars is desirable; its purpose is…

astro-ph.EP2026

Modelling the long-term impacts of artificial warming on the Martian water cycle and surface ice distribution

Ashwin S. Braude, Edwin S. Kite, Mark I. Richardson +2

Recent papers by Ansari et al. (2024, Science Advances 10, eadn4650) and Richardson et al. (2025, arXiv eprint 2504.01455) have suggested that global warming of the Martian surface…

physics.ao-ph2022★ 3 cited

Pyrocast: a Machine Learning Pipeline to Forecast Pyrocumulonimbus (PyroCb) Clouds

Kenza Tazi, Emiliano Díaz Salas-Porras, Ashwin Braude +5

Pyrocumulonimbus (pyroCb) clouds are storm clouds generated by extreme wildfires. PyroCbs are associated with unpredictable, and therefore dangerous, wildfire spread. They can also…

stat.ML2022★ 3 cited

Identifying the Causes of Pyrocumulonimbus (PyroCb)

Emiliano Díaz Salas-Porras, Kenza Tazi, Ashwin Braude +5

A first causal discovery analysis from observational data of pyroCb (storm clouds generated from extreme wildfires) is presented. Invariant Causal Prediction was used to develop to…

astro-ph.EP2021★ 13 cited

No detection of SO2, H2S, or OCS in the atmosphere of Mars from the first two Martian years of observations from TGO/ACS

Ashwin S. Braude, F. Montmessin, K. S. Olsen +13

The detection of sulphur species in the Martian atmosphere would be a strong indicator of volcanic outgassing from the surface of Mars. We wish to establish the presence of SO2, H2…

astro-ph.EP2019★ 37 cited

Colour and Tropospheric Cloud Structure of Jupiter from MUSE/VLT: Retrieving a Universal Chromophore

Ashwin S. Braude, Patrick G. J. Irwin, Glenn S. Orton +1

Recent work by Sromovsky et al. (2017, Icarus 291, 232-244) suggested that all red colour in Jupiter's atmosphere could be explained by a single colour-carrying compound, a so-call…

astro-ph.EP2019★ 44 cited

Latitudinal variation in the abundance of methane (CH4) above the clouds in Neptune's atmosphere from VLT/MUSE Narrow Field Mode Observations

Patrick G. J. Irwin, Daniel Toledo, Ashwin S. Braude +5

Observations of Neptune, made in 2018 using the new Narrow Field Adaptive Optics mode of the Multi Unit Spectroscopic Explorer (MUSE) instrument at the Very Large Telescope (VLT) f…

astro-ph.EP2018★ 22 cited

Analysis of gaseous ammonia (NH) absorption in the visible spectrum of Jupiter - Update

Patrick G. J. Irwin, Neil Bowles, Ashwin S. Braude +5

An analysis of currently available ammonia (NH) visible-to-near-infrared gas absorption data was recently undertaken by Irwin et al. (Icarus, 302 (2018) 426) to help interpret…