Loading...
I am an oceanographer and climate scientist. I am a Senior Scientist in the Climate Mitigtion team at the UK Met Office, where I study global and regional climate change under various greenhouse gas emission scenarios using reduced-complexity climate models.
Prior to joining the Met Office, I was a Postdoctoral Research Associate with Prof Ric Williams at the University of Liverpool, UK and was a Postdoctoral Researcher with Dr Stephen Griffies at Princeton University, USA. I completed my PhD from Imperial College London, UK, where I worked with Prof Pavel Berloff.
For more details on my professional life, see my Curriculum Vitae [Last updated Jan 2026].
My research primarily focuses on the ocean's role in the climate system. I am interested in questions pertaining to climate variability and predictability, meridional overturning circulation and tracer transport, mesoscale-submesoscale processes and turbulence. My interests also include the use of reduced-complexity climate models or climate emulators for climate projections and assessing climate change impacts.I use a combination of theoretical frameworks, idealised models, climate model outputs and observations in my research.
Below are short summaries of my research interests and past work.
Both long‑term changes in Earth’s climate and interannual–multidecadal climate fluctuations — driven by human activities and natural variability in the climate system — shape regional climates and influence climate extremes. Improving the understanding and predictability of these signals is crucial for effective climate mitigation and adaptation. My interests are in,
The Atlantic Meridional Overturning Circulation (AMOC) involves a northward flow of warm water near the surface and a southward flow of cold, deep water in the Atlantic Ocean. This circulation significantly influences ocean temperatures and regional climates. I am interested in various aspects of the AMOC,
Ocean mesoscale-submesoscale eddies, typically ranging from 1 to 100 kilometers in size, are crucial for large-scale circulation, ocean transport and mixing. Ocean eddies primarily form through baroclinic instability, a process by which potential energy is converted into kinetic energy in the ocean. My interests are in
Alternating jets have been well-observed in Earth's oceans and planetary atmospheres like Jupiter. The jets are formed due to intreactions between mesoscale eddies and Rossby waves. In the ocean, these jets are few hundreds to thousands of kilometres long and can stay for a few months to a couple of years. I am interested in various aspects of these jets,