S. Wannawichian

TL;DR: A large campaign of observations of these planets has been undertaken using the Hubble Space Telescope, in association with measurements from planetary spacecraft and solar wind conditions both propagated from 1 AU and measured near each planet as mentioned in this paper.

TL;DR: In this article, the authors report ultraviolet images of Saturn, which, when combined with simultaneous Cassini measurements of the solar wind and Saturn kilometric radio emission, demonstrate that its aurorae differ morphologically from those of both Earth and Jupiter.

TL;DR: In this article, the center of the auroral oval oscillates with period 10.76 h ± 0.15 h for both January 2007 and February 2008, i.e., close to the periods determined for oscillations in other magnetospheric phenomena.

TL;DR: For example, Nichols et al. as discussed by the authors showed that the radius of the northern auroral oval is 1.5 smaller than the southern, indicating that Saturn's polar ionospheric magnetic field, measured for the first time in the ionosphere, is � 17% larger in the north than the south.

TL;DR: In this paper, a search for Enceladus' auroral footprint using series of UV images of Saturn's aurora taken by the Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS) in January 2004 and the Advanced Camera for Surveys (ACS) between February 2005 and January 2007 was conducted.