Voyager era stereo images are used to map the geology and topography of Ra Patera (a major active volcanic center and possible site of sulfur eruptions on Io). The summit of Ra Patera reaches only approx.1 km above the surrounding plains. Pre-Voyager-era lava flows occur on slopes of 0.1-0.3 deg, comparable to the lunar mare. These flows were emplaced at either low viscosities, high eruption rates, or both. A 600- km-long ridged mountain unit (rising to approx. 8 km near Carancho Patera) forms a 60 by 90 km wide plateau approx. 0.5 km high 50 km east of Ra Patera. The new lava flows observed by Galileo flowed around the southern edge of this plateau
The morphology of volcanic features on Ganymede differs significantly from that on the terrestrial p...
In Sep. 1992, the Magellan spacecraft filled the final large gap in its coverage of Venus when it im...
This work examines lava emplacement processes by characterizing surface units using field and remote...
Ra Patera is a major active volcanic center on Io and a possible site of liquid sulfur eruptions. Vo...
Paterae (volcano-tectonic depressions) are among the most prominent topographic features on Io. They...
Geologic mapping of the Jovian satellite Io has been completed at 1:15,000,000 scale for an area lyi...
The Magellan spacecraft has mapped nearly 99% of the surface of Venus with high resolution synthetic...
We have completed a new 1:15,000,000 global geologic map of Jupiter's volcanic moon, Io, based on a ...
We are preparing a new global geo-logic map of Jupiter s volcanic moon, Io. Here we report the type ...
Linking quantitative measurements of lava fl ow surface morphology with historical observations of e...
A new global geologic map of Jupiter's volcanic moon, Io is being prepared, with the focus being on ...
Near-infrared observations of Io during occultation by Jupiter and the other Galilean satellites hav...
The Jovian moon Io hosts the most powerful persistently active volcano in the Solar System, Loki Pat...
The surface characteristics and morphology of the equatorial region of Venus were first described by...
Mapping of lava flows in unvegetated areas of active volcanoes using optical satellite data is chall...
The morphology of volcanic features on Ganymede differs significantly from that on the terrestrial p...
In Sep. 1992, the Magellan spacecraft filled the final large gap in its coverage of Venus when it im...
This work examines lava emplacement processes by characterizing surface units using field and remote...
Ra Patera is a major active volcanic center on Io and a possible site of liquid sulfur eruptions. Vo...
Paterae (volcano-tectonic depressions) are among the most prominent topographic features on Io. They...
Geologic mapping of the Jovian satellite Io has been completed at 1:15,000,000 scale for an area lyi...
The Magellan spacecraft has mapped nearly 99% of the surface of Venus with high resolution synthetic...
We have completed a new 1:15,000,000 global geologic map of Jupiter's volcanic moon, Io, based on a ...
We are preparing a new global geo-logic map of Jupiter s volcanic moon, Io. Here we report the type ...
Linking quantitative measurements of lava fl ow surface morphology with historical observations of e...
A new global geologic map of Jupiter's volcanic moon, Io is being prepared, with the focus being on ...
Near-infrared observations of Io during occultation by Jupiter and the other Galilean satellites hav...
The Jovian moon Io hosts the most powerful persistently active volcano in the Solar System, Loki Pat...
The surface characteristics and morphology of the equatorial region of Venus were first described by...
Mapping of lava flows in unvegetated areas of active volcanoes using optical satellite data is chall...
The morphology of volcanic features on Ganymede differs significantly from that on the terrestrial p...
In Sep. 1992, the Magellan spacecraft filled the final large gap in its coverage of Venus when it im...
This work examines lava emplacement processes by characterizing surface units using field and remote...