… We identify six new auroral detections of Uranus in post-equinox HST observations of 2012
… We suggest that near-equinoctial aurorae of Uranus might be pulsed cusp emissions formed …

… In the next subsection, we review the results of an attempt to observe compression-enhanced
auroras during the recent intensive Uranus HST campaign outlined in section 1. …

The aurorae of Uranus were recently detected in the far ultraviolet with the Hubble Space …
We analyze here two new HST Uranus campaigns executed in Sept. 2012 and Nov. 2014 with …

… When Uranus reached the reverse configuration between equinox and southern summer
solstice, in late 2017, HST tracked the planetary auroral response to unusually powerful solar …

… Uranus and its moons from pole to pole, and to view its ring system edge on. That opportunity
comes in 2007. By observing the Uranus system at equinox … position of the auroral zones, …

… Moreover, Uranus is now close to equinox, a situation radically different from solstice
conditions prevailing in 1986 (a Uranian revolution lasts 84 years), which has never been …

… only spacecraft encounter with Uranus, that of Voyager 2 in 1986. Fortunately, auroras at the
… , this approach is applied to improving the resolution of the magnetic field of Uranus. The …

… The equinox of Uranus occurred in late 2007 and these … 4 years after equinox, equivalent
to 15 of circumsolar rotation. … , and Uranus for the auroral and non-auroral regions (E Auroral …

… the relative importance of the auroral and non-auroral processes’. … the auroral process is in
driving H 3 + emission at Uranus. … temperature as Uranus moved away from equinox in 2007 …

… rotation for a Uranus-like configuration at equinox. The purpose here is not to produce
faithful simulations of Uranus but rather to investigate the effects of rotation on a Uranus-like …