A statistical analysis of the location and width of Saturns southern auroras
Characteristics of Saturns FUV aurora observed with the Space Telescope Imaging Spectrograph
Characteristics of Saturns polar atmosphere and auroral electrons derived from HST/STIS, FUSE and Cassini/UVIS spectra
Open flux in Saturns magnetosphere
Signatures of field-aligned currents in Saturns nightside magnetosphere
Survey of Saturn auroral storms observed by the Hubble Space Telescope: Implications for storm time scales
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2000-12-07T11:17:13Z/2000-12-08T13:41:49Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Prange comma Renee, 2007, 'FUV diagnostic of Saturn's stratosphere with STIS. Water influx from the ring and polar haze', 1.0, European Space Agency, https://doi.org/10.5270/esa-2xo41ev