Details

Autor(en) / Beteiligte

• Lamy, L.
• Prangé, R.
• Hansen, K. C.
• Tao, C.
• Cowley, S. W. H.
• Stallard, T. S.
• Melin, H.
• Achilleos, N.
• Guio, P.
• Badman, S. V.
• Kim, T.
• Pogorelov, N.

Titel

The aurorae of Uranus past equinox

Ist Teil von

• Journal of geophysical research. Space physics, 2017-04, Vol.122 (4), p.3997-4008

Ort / Verlag

Washington: Blackwell Publishing Ltd

Erscheinungsjahr

2017

Quelle

Wiley Online Library

Beschreibungen/Notizen

• 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. Key Points We identify six new auroral detections of Uranus in post‐equinox HST observations of 2012 and 2014 These emissions are bright extended southern spots corotating with the planet, consistent with pulsed cusp aurorae We retrieved the longitude of magnetic poles by fitting the auroral emissions with model auroral ovals