A phenomenological model of Ios UV aurora based on HST/STIS observations
Emission profiles of neutral oxygen and sulfur in Ios exospheric corona
High-resolution far ultraviolet spectrum of electron-excited SO2
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
Multi-wavelength simulations of atmospheric radiation from Io with a 3-D spherical-shell backward Monte Carlo radiative transfer model
Parallel Electron Beams at Io: Numerical Simulations of the Dense Plasma Wake
The Abundance of Atomic Sulfur in the Atmosphere of Io
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
1998-08-21T17:52:33Z/1998-08-27T20:18:17Z
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, Roesler comma Fred, 2006, 'Spatial & Temporal Variations in the UV Emission from the Atmosphere of Io', 1.0, European Space Agency, https://doi.org/10.5270/esa-a9oi7yj