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Identification of gaseous SO2 and new upper limits for other gases on Io

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TLDR
In this paper, the identification of gaseous sulfur dioxide on Io by Voyager 1 is reported, and preliminary upper limits for other atmospheric gases are presented, with a depletion of hydrogen, carbon and nitrogen.
Abstract
The identification of gaseous sulfur dioxide on Io by Voyager 1 is reported, and preliminary upper limits for other atmospheric gases are presented. Averaged spectra taken by the Voyager IRIS experiment in the range of 1,000 to 1,200/cm are interpreted as containing three fundamental sulfur dioxide bands, with intensities most nearly corresponding to an atmospheric model with a sulfur dioxide abundance of 0.2 cm atm. Upper limits for COS, CS2, SO3, H2S, CO2, O3, N2O, H2O, CH4, NH3 and HC1, not detected in the spectra, were calculated on the basis of the radiative transfer equation for temperatures of 130 and 250 K; a depletion of hydrogen, carbon and nitrogen is noted. It is suggested that a SO2 outgassing from a cooling sulfur extrusion is the major source of the observed atmospheric SO2.

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Infrared observations of the saturnian system from voyager 1.

TL;DR: During the passage of Voyager 1 through the Saturn system, the infrared instrument acquired spectral and radiometric data on Saturn, the rings, and Titan and other satellites, implying a depletion of helium in the atmosphere of Saturn relative to that of Jupiter.
Journal ArticleDOI

Nonlinear standing Alfvén wave current system at Io: Theory

TL;DR: In this article, a nonlinear analytical model of the Alfven current tubes continuing the currents through Io (or rather its ionosphere) generated by the unipolar inductor effect due to Io's motion relative to the magnetospheric plasma was presented.
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Direct plasma measurements in the Io torus and inner magnetosphere of Jupiter

TL;DR: In this article, the details of positive ion measurements made in the inner magnetosphere are discussed and an analysis of these measurements to obtain plasma composition, flow speeds, and temperatures is given.
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Overview of the Voyager ultraviolet spectrometry results through Jupiter encounter

TL;DR: The observations of a number of objects by the Voyager EUV instruments are summarized in this article, and the summary is considered to demonstrate the wide ranging application of the EUV spectroscopy and emphasizes the continuing importance of the search and discovery nature of spectroscopic techniques.
References
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Journal ArticleDOI

Melting of Io by Tidal Dissipation

TL;DR: The dissipation of tidal energy in Jupiter's satellite Io is likely to have melted a major fraction of the mass, and consequences of a largely molten interior may be evident in pictures of Io's surface returned by Voyager I.
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