A phenomenological model of Ios UV aurora based on HST/STIS observations
Constraints on Ios interior from auroral spot oscillations
Emission profiles of neutral oxygen and sulfur in Ios exospheric corona
Far-Ultraviolet Imaging Spectroscopy of Ios Atmosphere with HST/STIS
Hubble space telescope far-ultraviolet observations of Io: Determining atmospheric abundances, mapping the sulfur dioxide distribution, and correlating the molecular and atomic atmosphere
Ios aurora: HST/STIS observations
Ios auroral limb glow: Hubble Space Telescope FUV observations
Ios dayside SO 2 atmosphere
Ios SO2 atmosphere from HST Lyman-a images: 1997 to 2018
Lyman-a imaging of the SO2 distribution on Io
Model Calculations for Ios Atmosphere at Eastern and Western Elongations
Parallel Electron Beams at Io: Numerical Simulations of the Dense Plasma Wake
Simulation of Ios auroral emission: Constraints on the atmosphere in eclipse
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
1997-09-26T10:17:00Z/1997-10-14T06:30:18Z
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, Moos comma H. Warren, 2006, 'Spatial Distribution of Io's Extended UV Emissions', 1.0, European Space Agency, https://doi.org/10.5270/esa-ghdt10s