Area of research
Astronomy and Astrophysics · Aerospace Engineering
Research interest
Research focused on Uranus and Atmosphere (unit), with related work in Saturn, Ionosphere, Jupiter (rocket family). Notable publications include 'The science case for an orbital mission to Uranus: Exploring the origins and evolution of ice giant planets', 'Earth‐based detection of Uranus' aurorae', and 'Ice Giant Systems: The scientific potential of orbital missions to Uranus and Neptune'.
The atmosphere of Titan in late northern summer from JWST and Keck observations
Spatiotemporal Variations of Temperature in Jupiter’s Upper Atmosphere
Temporal Variability of the Northern Infrared Aurora of Jupiter as Captured by JWST
Pole‐to‐Pole Vertical Ionospheric Profiles at Jupiter From JWST
Temperature, Composition, and Cloud structure in Atmosphere of Uranus from MIRI-MRS and NIRSpec-IFU Spectra
Ionospheric irregularities at Jupiter observed by JWST
Saturn's Atmosphere in Northern Summer Revealed by JWST/MIRI
An Energetic Eruption With Associated SO 1.707 Micron Emissions at Io's Kanehekili Fluctus and a Brightening Event at Loki Patera Observed by JWST
Asymmetric Ionospheric Jets in Jupiter's Aurora
Global upper-atmospheric heating on Jupiter by the polar aurorae
Saturn's Weather‐Driven Aurorae Modulate Oscillations in the Magnetic Field and Radio Emissions
Ice Giant Systems: The scientific potential of orbital missions to Uranus and Neptune
The H <sub>3</sub> <sup>+</sup> ionosphere of Uranus: decades-long cooling and local-time morphology
Local-time averaged maps of H <sub>3</sub> <sup>+</sup> emission, temperature and ion winds
Observations of the chemical and thermal response of ‘ring rain’ on Saturn’s ionosphere
Identification of Jupiter’s magnetic equator through H3+ ionospheric emission
The quest for H$_3^+$ at Neptune: deep burn observations with NASA IRTF iSHELL
The Great Cold Spot in Jupiter's upper atmosphere
Heating of Jupiter’s upper atmosphere above the Great Red Spot
Ground-based observations of Saturn’s auroral ionosphere over three days: Trends in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si3.gif" overflow="scroll"><mml:mrow><mml:msubsup><mml:mrow><mml:mtext>H</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msubsup></mml:mrow></mml:math> temperature, density and emission with Saturn local time and planetary period oscillation
The science case for an orbital mission to Uranus: Exploring the origins and evolution of ice giant planets
Dynamic auroral storms on Saturn as observed by the Hubble Space Telescope
Saturn’s auroral morphology and field-aligned currents during a solar wind compression
Earth‐based detection of Uranus' aurorae
Rotational modulation and local time dependence of Saturn's infrared H<sub>3</sub><sup>+</sup> auroral intensity
Peak emission altitude of Saturn's H<sub>3</sub><sup>+</sup> aurora