Jupiter Publication Links: 

Jupiter Systems

• Tobiska, et al 2007 SET TR: Galileo UV observations of H Lyman-alpha in Jupiter’s low latitude upper atmosphere
• Pryor, et al 2005 Icarus: Cassini UVIS observations of auroral H2and H Lyman-α emissions
• Gladstone, et al 2004 PSS: Constraints on Jupiter’s hydrogen corona from Galileo UVS observations
• Pryor, et al 2001 SSR:  Remote Sensing of H from Ulysses and Galileo
• Ajello, et al 2001 Icarus:  EUV and FUV auroral spectra from Galileo EUVS (540 — 1280 Å) and HUT (830 — 1850 Å) observations
• Clarke, et al 1998 JGR:  Hubble imaging of Jupiter’s UV aurora during the Galileo mission
• Pryor, et al 1998 JGR:  Galileo UVS spectrum from 1600 – – 3200 Å
• Ajello, et al 1998 JGR:  Spectra from Galileo UVS (540 — 1280 Å) and EUVS (1130 — 4320 Å)
• Hord, et al 1992 SSR:  Description of the Galileo Ultraviolet Spectrometer and planned observations at Jupiter
• Bagenal, et al 1992 GRL: Radial profile of O++ abundance between 4.0 and 42 RJ based on Voyager 1 data
• Shemansky and Judge 1988 JGR: Comparison of Voyager data with earlier Pioneer 10 and rocket observations
• Shemansky 1985 JGR:  Mechanism for the H Ly-α bulge in EUV equatorial emission
• McConnell, et al 1982 PSS:  Photochemical model with vertical transport of ions
• Brown and Shemansky 1982 APJ:  Ion-ion and ion-atom reactions may determine the structure of Jupiter’s hot plasma torus
• Festou, et al 1981 JGR:  Analysis of stellar occultation observed by Voyager 2
• Cook, et al 1981 JGR:  Aurora in darkside Voyager I images at least partially attributed to lo torus aurora
• Broadfoot, et al 1981 JGR:  Summary of Voyager UVS observations from the 1977 launch through the 25 March 1979 Jupiter encounter 
• Sandel, et al 1979 Science:  Voyager 2 encounter with Jupiter
• Broadfoot, et al 1979 Science:  Voyager 1 encounter with Jupiter 
• Broadfoot, et al 1977 SSR:  Description of the Voyager Ultraviolet Spectrometer and planned observations

Jupiter Systems – Io

• Taylor, et al 1995 JGR:  Model of EUV Io plasma torus emission developed using Voyager 1 in situ and remote observations
• Hall 1994 APJ:  370 to 735 Å spectrum from the Extreme Ultraviolet Explorer (EUVE)
• Schneider, et al 1991 Science:  Sodium-bearing molecules interacting with the lo plasma torus may be the source of fast neutral sodium
• Shemansky 1988 JGR:  Neutral cloud theory does not support observed ion partitioning
• Shemansky 1987 JGR:  Model of collisional diffusive equilibrium in the lo plasma torus and comparison to Voyager UVS data
• Smyth and Shemansky 1983 APJ:  Model of the escape of atomic oxygen from lo and its distribution in the Jupiter magnetosphere
• Brown, et al 1983 APJ:  Effects of fast ion-ion and ion-atom reactions on chemistry in the Io plasma torus
• Shemansky and Sandel 1982 JGR:  Electron-electron heating appears to be the dominant mechanism transporting energy to the plasma
• Shemansky 1980 APJ:  Calculation of limits on ion mass-loading and diffusion-loss rates
• Shemansky 1980 APJ:  Calculations of radiative cooling efficiencies and predicted line intensities for species in the torus

Jupiter Systems – Europa

• Hansen, et al 2005 Icarus:  Cassini UVIS observes atomic oxygen atmosphere at Europa