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Asymmetric Ionospheric Jets in Jupiter's Aurora

Wang, Ruoyan; Stallard, Tom S; Melin, Henrik; Baines, Kevin H; Achilleos, Nicholas; Rymer, Abigail M; Ray, Licia C; ... Miller, Steve; + view all (2023) Asymmetric Ionospheric Jets in Jupiter's Aurora. JGR: Space Physics , 128 (12) , Article e2023JA031861. 10.1029/2023JA031861. Green open access

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Abstract

Simultaneous infrared observations of (Formula presented.) and H2 emissions from Jupiter's northern aurora using the Near Infrared Spectrograph at Keck Observatory were used to measure the ionospheric and thermospheric wind velocities. (Formula presented.) ions supercorotate near the dawn auroral oval and subcorotate across the dusk sector and in the dawn polar region relative to the planetary rotation rate, broadly in agreement with past observations and models. An anticyclonic vortex is discovered in H2 flows, closely matching the mean magnetospheric subcorotation when the observed magnetospheric flows are averaged azimuthally. In comparing ion and neutral winds, we measure the line-of-sight effective ion drift in the neutral reference frame for the first time, revealing two blue-shifted sunward flows of ∼2 km/s. Observed (Formula presented.) and H2 emissions overlap with predictions of the Pedersen conductivity layer, suggesting two different regions of the ionosphere: (a) a deep layer, where neutral forces dominate the thermosphere and symmetric breakdown-in-corotation currents can close, and (b) a higher layer, where the observed effective ion drift allows dawn-to-dusk Pedersen currents within the upper atmosphere, in turn closing asymmetric currents within the magnetosphere. This ionospheric structure aligns well with recent Juno observations of Jupiter's aurora. The detected thermospheric vortex implies the driving of neutral flows by the momentum from the magnetosphere within the thermosphere and deeper in the atmosphere to potentially 20 mbar. Jovian neutral thermosphere might bridge the gap between current observations and modelings and perhaps be significant to the dynamics of aurora on Earth and other outer planets.

Type: Article
Title: Asymmetric Ionospheric Jets in Jupiter's Aurora
Open access status: An open access version is available from UCL Discovery
DOI: 10.1029/2023JA031861
Publisher version: https://doi.org/10.1029/2023JA031861
Language: English
Additional information: Copyright © 2023. The Authors. This is an open access article under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs License, https://creativecommons.org/licenses/by-nc-nd/4.0/, which permits use and distribution in any medium, provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made.
Keywords: Jupiter; infrared; aurora; ion and neutral wind; ionosphere; magnetosphere
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10183264
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