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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

Advanced Net Flux Radiometer for the Ice Giants

Space Science Reviews Springer 216 (2020) 11

Authors:

S Aslam, RK Achterberg, SB Calcutt, V Cottini, NJ Gorius, T Hewagama, PG Irwin, CA Nixon, G Quilligan, M Roos-Serote, AA Simon, D Tran, G Villanueva

Abstract:

The design of an advanced Net Flux Radiometer (NFR), for inclusion as a payload on a future Ice Giants probe mission, is given. The Ice Giants NFR (IG-NFR) will measure the upward and downward radiation flux (hence net radiation flux), in seven spectral bands, spanning the range from solar to far infra-red wavelengths, each with a 5° Field-Of-View (FOV) and in five sequential view angles (±80°, ±45°, and 0°) as a function of altitude. IG-NFR measurements within either Uranus or Neptune’s atmospheres, using dedicated spectral filter bands will help derive radiative heating and cooling profiles, and will significantly contribute to our understanding of the planet’s atmospheric heat balance and structure, tropospheric 3-D flow, and compositions and opacities of the cloud layers. The IG-NFR uses an array of non-imaging Winston cones integrated to a matched thermopile detector Focal Plane Assembly (FPA), with individual bandpass filters, housed in a diamond windowed vacuum micro-vessel. The FPA thermopile detector signals are read out in parallel mode, amplified and processed by a multi-channel digitizer application specific integrated circuit (MCD ASIC) under field programmable gate array (FPGA) control. The vacuum micro-vessel rotates providing chopping between FOV’s of upward and downward radiation fluxes. This unique design allows for small net flux measurements in the presence of large ambient fluxes and rapidly changing ambient temperatures during the probe descent to ≥10 bar pressure.

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Uranus in Northern Midspring: Persistent Atmospheric Temperatures and Circulations Inferred from Thermal Imaging

The Astronomical Journal American Astronomical Society 159:2 (2020) 45-45

Authors:

Michael T Roman, Leigh N Fletcher, Glenn S Orton, Naomi Rowe-Gurney, Patrick GJ Irwin
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Stormy water on Mars: The distribution and saturation of atmospheric water during the dusty season

Science American Association for the Advancement of Science (AAAS) (2020) eaay9522-eaay9522

Authors:

Anna A Fedorova, Franck Montmessin, Oleg Korablev, Mikhail Luginin, Alexander Trokhimovskiy, Denis A Belyaev, Nikolay I Ignatiev, Franck Lefèvre, Juan Alday, Patrick GJ Irwin, Kevin S Olsen, Jean-Loup Bertaux, Ehouarn Millour, Anni Määttänen, Alexey Shakun, Alexey V Grigoriev, Andrey Patrakeev, Svyatoslav Korsa, Nikita Kokonkov, Lucio Baggio, Francois Forget, Colin F Wilson

Abstract:

The loss of water from Mars to space is thought to result from the transport of water to the upper atmosphere, where it is dissociated to hydrogen and escapes the planet. Recent observations have suggested large, rapid seasonal intrusions of water into the upper atmosphere, boosting the hydrogen abundance. We use the Atmospheric Chemistry Suite on the ExoMars Trace Gas Orbiter to characterize the water distribution by altitude. Water profiles during the 2018–2019 southern spring and summer stormy seasons show that high-altitude water is preferentially supplied close to perihelion, and supersaturation occurs even when clouds are present. This implies that the potential for water to escape from Mars is higher than previously thought.
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Towards the analysis of JWST exoplanet spectra: the effective temperature in the context of direct imaging

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 490:2 (2019) 2086-2090

Authors:

Jean-Loup Baudino, J Taylor, PGJ Irwin, R Garland

Abstract:

ABSTRACT The current sparse wavelength range coverage of exoplanet direct imaging observations, and the fact that models are defined using a finite wavelength range, lead both to uncertainties on effective temperature determination. We study these effects using blackbodies and atmospheric models and we detail how to infer this parameter. Through highlighting the key wavelength coverage that allows for a more accurate representation of the effective temperature, our analysis can be used to mitigate or manage extra uncertainties being added in the analysis from the models. We find that the wavelength range coverage will soon no longer be a problem. An effective temperature computed by integrating the spectroscopic observations of the James Webb Space Telescope will give uncertainties similar to, or better than, the current state–of–the–art, which is to fit models to data. Accurately calculating the effective temperature will help to improve current modelling approaches. Obtaining an independent and precise estimation of this crucial parameter will help the benchmarking process to identify the best practice to model exoplanet atmospheres.
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Constraints on Uranus's haze structure, formation and transport

Icarus Elsevier BV 333 (2019) 1-11

Authors:

Daniel Toledo, Patrick GJ Irwin, Pascal Rannou, Nicholas A Teanby, Amy A Simon, Michael H Wong, Glenn S Orton
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