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Juno Jupiter image

Prof. Patrick Irwin

Professor of Planetary Physics

Research theme

  • Exoplanets and planetary physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Exoplanet atmospheres
  • Planetary atmosphere observation analysis
  • Solar system
patrick.irwin@physics.ox.ac.uk
Telephone: 01865 (2)72083
Atmospheric Physics Clarendon Laboratory, room 306
Personal research page
NEMESIS
Github data sharing website
  • About
  • Publications

Constraints on aerosol structure and formation in the atmosphere of the ice giants from microphysics simulations

Copernicus Publications (2024)

Authors:

Daniel Toledo, Patrick Irwin, Pascal Rannou, Leigh Fletcher, Margarita Yela
More details from the publisher

Detection of Cyclopropenylidene on Titan

Copernicus Publications (2024)

Authors:

Conor Nixon, Alexander Thelen, Martin Cordiner, Zbigniew Kisiel, Steven Charnley, Edward Molter, Joseph Serigano, Patrick Irwin, Nicholas Teanby, Yi-Jehng Kuan
More details from the publisher

Ice lines and the formation of Uranus and Neptune

Copernicus Publications (2024)

Authors:

Olivier Mousis, Artyom Aguichine, Ravit Helled, Patrick Irwin, Jonathan I Lunine
More details from the publisher

Ice-Giants Net Flux Radiometer for Heat Flux Measurements

Copernicus Publications (2024)

Authors:

Shahid Aslam, Simon Calcutt, Nicolas Gorius, Patrick Irwin, George Nehmetallah, Gerard Quilligan, Dat Tran
More details from the publisher

Isotopic composition of water vapour in the Martian atmosphere: vertical profiles from ACS MIR on ExoMars TGO

Copernicus Publications (2024)

Authors:

Juan Alday, Patrick GJ Irwin, Colin F Wilson, Kevin S Olsen, Lucio Baggio, Franck Montmessin, Oleg Korablev, Alexander Trokhimovskiy, Anna A Fedorova, Denis A Belyaev, Alexey Shakun, Andrew Patrakeev, Alexey Grigoriev

Abstract:

We report retrievals in the 2.53 – 2.79 μm spectral range using the Atmopheric Chemistry Suite onboard of ExoMars Trace Gas Orbiter, which allow the simultaneous measurement of vertical profiles of H and O isotope ratios in water vapour in the Martian atmosphere. The large coverage of ACS MIR solar occultations provides the possibility to analyse the spatial, seasonal and diurnal variations of these ratios.
More details from the publisher
Details from ORA

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