Auroral and Non‐Auroral H <sub>3</sub> <sup>+</sup> Ion Winds at Uranus With Keck‐NIRSPEC and IRTF‐iSHELL

Abstract To date, no investigation has documented ionospheric flows at Uranus. Previous investigations of Jupiter and Saturn have demonstrated that mapping ion winds can be used to understand ionospheric currents and how these connect to magnetosphere‐ionosphere coupling. We present a study of Uranus's near infrared emissions (NIR) using data from the Keck II Telescope's Near InfraRed SPECtrograph (NIRSPEC) and the InfraRed Telescope Facility's iSHELL spectrograph. H 3 + emission lines were used to derive dawn‐to‐dusk intensity, ionospheric temperatures and ion densities to identify auroral emissions, with their Doppler shifts used to measure ion velocities. We confirm the presence of the southern NIR aurora in 2016, driven by elevated H 3 + column densities up to 6.0 × 10 16 m −2 . While no auroral emissions were detected in 2014, we find a 14%–20% super rotation across the planet's disk in 2014 and a 7%–18% super rotation in 2016.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-04-01
DOI
https://doi.org/10.1029/2024gl112001
Citations
2
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
2.31

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article

Auroral and Non‐Auroral H 3 + Ion Winds at Uranus With Keck‐NIRSPEC and IRTF‐iSHELL

James O’Donoghue, Emma Thomas, M. N. Chowdhury, Luke Moore et al.
2 citations
Geophysical Research Letters
Astro and Planetary Science
2.31
article

Auroral and Non‐Auroral H 3 + Ion Winds at Uranus With Keck‐NIRSPEC and IRTF‐iSHELL

James O’Donoghue, Emma Thomas, M. N. Chowdhury, Luke Moore, Hideyo Kawakita, Ruoyan Wang, Katie Knowles, Ronald J. Vervack, Tom Stallard, Neil Dello Russo, R. E. Johnson, Henrik Melin, Paola Tiranti
article en
2 citations

Abstract

Abstract To date, no investigation has documented ionospheric flows at Uranus. Previous investigations of Jupiter and Saturn have demonstrated that mapping ion winds can be used to understand ionospheric currents and how these connect to magnetosphere‐ionosphere coupling. We present a study of Uranus's near infrared emissions (NIR) using data from the Keck II Telescope's Near InfraRed SPECtrograph (NIRSPEC) and the InfraRed Telescope Facility's iSHELL spectrograph. H 3 + emission lines were used to derive dawn‐to‐dusk intensity, ionospheric temperatures and ion densities to identify auroral emissions, with their Doppler shifts used to measure ion velocities. We confirm the presence of the southern NIR aurora in 2016, driven by elevated H 3 + column densities up to 6.0 × 10 16 m −2 . While no auroral emissions were detected in 2014, we find a 14%–20% super rotation across the planet's disk in 2014 and a 7%–18% super rotation in 2016.

Geophysical Research LettersVol. 52(7)
Boston University (US), University of Leicester (GB), Aberystwyth University (GB), Kyoto Sangyo University (JP), Johns Hopkins University Applied Physics Laboratory (US), Northumbria University (GB), University of Reading (GB)
University of Leicester, Office of Nuclear Energy, Natural Environment Research Council, Science and Technology Facilities Council, Planetary Science Division, British Antarctic Survey
Openalex Percentile: Top 12%
Astro and Planetary Science
2.31
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