Rhian Chapman

I started at CEH in June 2018 with a background in modelling planetary climates, atmospheres, and surface-atmosphere interactions. I have experience in numerical modelling, computer programming and analysis of large data sets.

I completed my PhD in Planetary Science, studying the atmosphere of Mars. I ran computer experiments focused on surface dust lifting processes, their representation within the UK Mars Global Circulation Model (MGCM), and the potential impact of near-surface atmospheric dust phenomena on future Mars lander missions.
UKCEH - Hydro-Climate Risks
Member (Staff)