Auroral and Non-Auroral H3+ ion winds at Uranus with Keck-NIRSPEC and IRTF-iSHELL

Emma Miriam Thomas, Tom S. Stallard, Henrik Melin, Mohammad Nahid Chowdhury, Luke Moore, James O'Donoghue, Rosie Eleanor Johnson, Ruoyan Wang, Katie Louise Knowles, Paola Ines Tiranti, Neil Dello Russo, Ronald J. Vervack, Hideyo Kawakita

Research output: Working paperPreprint

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. H3+ 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 H3+ column densities up to 6.0 x 1016 m-2. While no auroral emissions were detected in 2014, we find a 14% to 20% super rotation across the planet’s disk in 2014 and a 7% to 18% super rotation in 2016.
Original languageEnglish
PublisherESS Open Archive
DOIs
Publication statusPublished - 28 Nov 2024

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