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Characteristics of Saturn's FUV aurora observed with the Space Telescope Imaging Spectrograph
DOI: 10.1029/2004JA010513 Bibcode: 2004JGRA..109.9207G

Trauger, John T.; Gustin, Jacques; Clarke, John T. +3 more

We analyze a set of 15 FUV images obtained between October 1997 and January 2001 with the Hubble Space Telescope Imaging Spectrograph (STIS), providing a good view of Saturn's south auroral oval. It is found that the morphology and brightness distribution of the aurora are dynamical with variations occurring on time scales of hours or less. The da…

2004 Journal of Geophysical Research (Space Physics)
eHST 80
Energy-flux relationship in the FUV Jovian aurora deduced from HST-STIS spectral observations
DOI: 10.1029/2003JA010365 Bibcode: 2004JGRA..10910205G

Clarke, J. T.; Cowley, S. W. H.; Grodent, D. +3 more

Far ultraviolet spectral observations of the Jovian aurora have been made since 1997 with the Space Telescope Imaging Spectrograph (STIS) on board the Hubble Space Telescope at low spectral resolution. The combination of the spectral resolution with the intensity variation along the STIS slit provides information on the latitudinal variation of th…

2004 Journal of Geophysical Research (Space Physics)
eHST 56
A possible auroral signature of a magnetotail reconnection process on Jupiter
DOI: 10.1029/2003JA010341 Bibcode: 2004JGRA..109.5201G

Clarke, J. T.; Waite, J. H.; Grodent, D. +2 more

Several theoretical models and in situ observations consistently suggest that the process of nightside reconnection associated with Earth's magnetospheric substorms is also taking place in the midnight tail region of Jupiter. We report the observation of a new auroral feature which takes the form of isolated spots appearing near the northern dusk-…

2004 Journal of Geophysical Research (Space Physics)
eHST 56
High-resolution far ultraviolet spectrum of electron-excited SO2
DOI: 10.1029/2003JA009828 Bibcode: 2004JGRA..109.2310V

Ajello, Joseph; Bhardwaj, Anil; Vatti Palle, Prahlad

The high-resolution UV capabilities (λ/Δλ = 105) of the Hubble Space Telescope (HST) equipped with the Space Telescope Imaging Spectrograph (STIS) reflects a need for a high-resolution laboratory UV spectral data base for comparison with observation. For the purpose of interpreting the astronomical observations of Io by HST the electron…

2004 Journal of Geophysical Research (Space Physics)
eHST 9