Io: Near infrared absorptions not attributable to SO(sub 2)
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Io Galilean satellites spectroscopy remote sensing↗
Engineering topics
Carlson, R.
Publications and source records attributed to Carlson, R..
Contemporaneous spectral imaging of Jupiter by Cassini/VIMS and Galileo/NIMS: latest science results
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Cassini VIMS Galileo NIMS Jupiter↗
Radiolysis processes on Europa
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Jupiter satellites composition↗
Contemporaneous spectral imaging of Jupiter by Galileo/NIMS and Cassini/VIMS: preliminary science results
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Jupiter Cassini VIMS Galileo NIMS↗
Io's diverse styles of volcanic activity: Results from Galileo NIMS
The Near-Infrared Mapping Spectrometer on Galileo has observed Io since June 1996. In 1999 and 2000, the spacecraft made three close fly-bys to Io, revealing for the first time, the detailed thermal structure of some of Io's hot spots.
Io↗
The toughest part of the road to Pluto
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Pluto JPL Europa Orbiter↗
Infrared Spectral Signatures for Io's Dark and Green Spots
This spectral study of Io identifies the infrared components of the visible spectral units (green and dark) as identified by Galileo. The green units possess sulfur dioxide and the dark units are associated with infrared thermal signatures. Additional information is contained in the original extended abstract.
Granahan, J. C.↗
Io's Diverse Styles of Volcanic Activity: Results from Galileo NIMS
Observations by Galileo's Near-Infrared Mapping Spectrometer were used to map the thermal structure of several of Io's hot spots, revealing different styles of volcanism Additional information is contained in the original extended abstract..
Lopes, R. M. C.↗
Dynamics and Evolution of SO2 Gas Condensation Around Prometheus-like Volcanic Plumes on Io as Seen by the Near Infrared Mapping Spectrometer
Near Infrared Mapping Spectrometer data acquired during the I24, 25, and 27 Io's Fly-bys by Galileo are analyzed to map the SO2 frost abundance and granularity. This allows a better understanding of the dynamics and evolution of gas condensation around volcanic plumes. Additional information is contained in the original extended abstract.
Doute, S.↗
Water Ice Grain Size Variations on Europa
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Europa Jovia Satellites Planetary Geology remote s↗
Silicate cooling model fits to Galileo NIMS data of volcanism on IO
The Near Infrared Mapping Spectrometer (NIMS) has obtained spectra of volcanoes on the surface of the jovian satellite Io.
Thermal emission lava flow active volcanism sulfur↗
Galileo NIMS Observations of Europa
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Europa Galileo Mission remote sensing Jovian Satel↗
Spectral Mapping of the Galilean Satellites
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Galilean mapping remote sensing infrared satellite↗
Galileo at IO: Results from the Near-Infrared Mapping Spectrometer
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IO Galileo volcanos↗
Active volcanism on Io: results from Galileo
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IO Galileo Volcanos↗
Wet and Dry Regions in Jupiter's Atmosphere
Models of Jupiter's formation and interior predict that its atmosphere is enriched in oxygen relative to the Sun and that consequently, a water cloud is present globally near the 5-bar pressure level.
Jupiter Atmosphere Water↗
Io as viewed by Galileo's Near-Infrared Mapping Spectrometer
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Io↗
A close-up look at Io from Galileo's Near-Infrared Mapping Spectrometer
Infrared spectral images of Jupiter's volcanic moon Io, acquired during October and November 1999 flybys of the Galileo spacecraft, were used to study the thermal structure and sulfur dioxide distribution of active volcanos.
IO↗