Physics
Scientific paper
Mar 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996lpi....27.1171s&link_type=abstract
Lunar and Planetary Science, volume 27, page 1171
Physics
2
Juno Dorsum, Magellan, Rifting, Venus, Volcanism
Scientific paper
Magellan image and altimetry data provide a basis to assess the geology and structure of many surface features on Venus. To understand how the processes of extension and volcanism are related, along with characterizing the styles and types of lava emplacement on Venus, the area between latitudes 25 degrees S and 50 degrees S and longitudes 90 degrees E and 120 degrees E, the Juno Dorsum Quadrangle (V-47) is being mapped. The Juno Region is bound by the upland of Aphrodite to the north, Artemis Corona to the east and Anio Planitia to the south and west. By using both spatial and temporal information from mapping, a basis is provided to understanding the relation between crustal stretching, rifting, and volcanism on Venus.
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