Preliminary analysis of Dione Regio, Venus: The final Magellan regional imaging gap

Details Preliminary analysis of Dione Regio, Venus: The final Magellan regional imaging gap Preliminary analysis of Dione Regio, Venus: The final Magellan regional imaging gap

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lpi....24..771k&link_type=abstract

In Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 2: G-M p 771-772 (SEE N94-16173 03-91)

Physics

Highlands, Planetary Geology, Venus Surface, Volcanoes, Imaging Techniques, Magellan Project (Nasa), Venus (Planet)

Scientific paper

In Sep. 1992, the Magellan spacecraft filled the final large gap in its coverage of Venus when it imaged an area west of Alpha Regio. F-BIDR's and some test MIDR's of parts of this area were available as of late December. Dione Regio was imaged by the Arecibo observatory and a preliminary investigation of Magellan images supports the interpretations made based on these earlier images: Dione Regio is a regional highland on which is superposed three large, very distinct volcanic edifices. The superior resolution and different viewing geometry of the Magellan images also clarified some uncertainties and revealed fascinating details about this region.

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