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On the origin of Saturn's outer auroral emission
DOI: 10.1029/2009JA014901 Bibcode: 2010JGRA..115.8219G

Gérard, Jean-Claude; Grodent, Denis; Radioti, Aikaterini +1 more

Ultraviolet Hubble Space Telescope images reveal a faint but distinct auroral emission equatorward of the main ring of emission of Saturn's southern polar region. This outer auroral emission is only visible near the nightside limb for the strongly tilted viewing geometry achieved in January 2004. We model the limb-brightening amplification of this…

2010 Journal of Geophysical Research (Space Physics)
Cassini eHST 44
Ten years of Hubble Space Telescope observations of the variation of the Jovian satellites' auroral footprint brightness
DOI: 10.1029/2009JA014456 Bibcode: 2010JGRA..115.2206W

Nichols, J. D.; Clarke, J. T.; Wannawichian, S.

During the past decade, FUV imaging of Jupiter's auroral region by the Hubble Space Telescope (HST) using two instruments, the Space Telescope Imaging Spectrograph (STIS) and the Advanced Camera for Surveys (ACS), has provided detailed information on the electrodynamic interaction between Io's, Ganymede's, and Europa's atmospheres and plasma in Ju…

2010 Journal of Geophysical Research (Space Physics)
eHST 32
Auroral signatures of flow bursts released during magnetotail reconnection at Jupiter
DOI: 10.1029/2009JA014844 Bibcode: 2010JGRA..115.7214R

Bonfond, B.; Gérard, J. -C.; Grodent, D. +1 more

Recent studies based on Hubble Space Telescope (HST) data reported the presence of transient polar dawn spots in the Jovian auroral region and interpreted them as signatures of internally driven magnetic reconnection in the Jovian magnetotail. Even though an association of the polar dawn spots with the reconnection process has been suggested, it h…

2010 Journal of Geophysical Research (Space Physics)
eHST 28
The 3-D extent of the Io UV footprint on Jupiter
DOI: 10.1029/2010JA015475 Bibcode: 2010JGRA..115.9217B

Bonfond, B.

The Io footprint (IFP) is the auroral signature of the electromagnetic interaction between Io and Jupiter's magnetosphere. It consists of several spots followed by an extended tail, which are located close to the feet of the magnetic field lines connecting Io to Jupiter. The size of the main spot is a controversial issue, and previously published …

2010 Journal of Geophysical Research (Space Physics)
eHST 25