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Senske et al. 1991
Senske, D.A., Head, J.W., Stofan, E.R. and Campbell, D.B. (1991). Geology and structure of Beta Regio, Venus: Results from Arecibo Radar Imaging. Geophysical Research Letters 18: doi: 10.1029/91GL01001. issn: 0094-8276.

Arecibo radar images of a portion of the equatorial region of Venus provide the first high resolution (1.5-- to 2.0-- km) synoptic coverage of Beta Regio. Within this area, tesseara, a complex deformed terrain, is identified as a major geologic unit with the largest region corresponding to a plateau on the east flank of the highland. Three models are proposed to explain the origin and evolution of Beta Regio and are identified as Mantle Plume/Passive Crust, Mantle Plume/Active Crust, and Mantle Plume/Crustal Spreading. The mantle Plume/Passive Crust model appears to be the most consistent with the geology in this region and suggests that a plume disrupts a preexisting region of tessera. ¿American Geophysical Union 1991

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Abstract

Keywords
Planetology, Solid Surface Planets and Satellites, Interiors, Planetology, Solid Surface Planets and Satellites, Surfaces, Planetology, Solid Surface Planets and Satellites, Tectonics, Planetology, Solid Surface Planets and Satellites, Volcanism
Journal
Geophysical Research Letters
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Publisher
American Geophysical Union
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