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Preliminary analysis of Dione Regio, Venus: The final Magellan regional imaging gapIn 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.
Document ID
19940011829
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Keddie, S. T.
(Brown Univ. Providence, RI, United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1993
Publication Information
Publication: Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 2: G-M
Subject Category
Lunar And Planetary Exploration
Accession Number
94N16302
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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