UCL Discovery
UCL home » Library Services » Electronic resources » UCL Discovery

The aurorae of Uranus past equinox

Lamy, L; Prange, R; Hansen, KC; Tao, C; Cowley, SWH; Stallard, TS; Melin, H; ... Pogorelov, N; + view all (2017) The aurorae of Uranus past equinox. Journal of Geophysical Research: Space Physics , 122 (4) pp. 3997-4008. 10.1002/2017JA023918. Green open access

[thumbnail of Guio_Lamy_et_al-2017-Journal_of_Geophysical_Research-_Space_Physics.pdf]
Preview
Text
Guio_Lamy_et_al-2017-Journal_of_Geophysical_Research-_Space_Physics.pdf - Published Version

Download (3MB) | Preview

Abstract

The aurorae of Uranus were recently detected in the far ultraviolet with the Hubble Space Telescope (HST) providing a new, so far unique, means to remotely study the asymmetric Uranian magnetosphere from Earth. We analyze here two new HST Uranus campaigns executed in September 2012 and November 2014 with different temporal coverage and under variable solar wind conditions numerically predicted by three different MHD codes. Overall, the HST images taken with the Space Telescope Imaging Spectrograph reveal auroral emissions in three pairs of successive images (one pair acquired in 2012 and two in 2014), hence 6 additional auroral detections in total, including the most intense Uranian aurorae ever seen with HST. The detected emissions occur close the expected arrival of interplanetary shocks. They appear as extended spots at southern latitudes, rotating with the planet. They radiate 5–24 kR and 1.3-8.8 GW of ultraviolet emission from H2, last for tens of minutes and vary on timescales down to a few seconds. Fitting the 2014 observations with model auroral ovals constrains the longitude of the southern (northern) magnetic pole to 104 ± 26° (284 ± 26°) in the Uranian Longitude System. We suggest that the Uranian near-equinoctial aurorae are pulsed cusp emissions possibly triggered by large-scale magnetospheric compressions.

Type: Article
Title: The aurorae of Uranus past equinox
Open access status: An open access version is available from UCL Discovery
DOI: 10.1002/2017JA023918
Publisher version: http://doi.org/10.1002/2017JA023918
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions.
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.ucl.ac.uk/id/eprint/1547249
Downloads since deposit
56Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item