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- W249848954 abstract "One key to understanding the history of resurfacing on Venus is better constraints on the emplacement timescales for the range of volcanic features visible on the surface. A figure shows a Magellan radar image and topography for a putative lava dome on Venus. 175 such domes have been identified with diameters ranging from 19 - 94 km, and estimated thicknesses as great as 4 km. These domes are thought to be volcanic in origin and to have formed by the flow of viscous fluid (i.e., lava) on the surface." @default.
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- W249848954 date "2012-03-12" @default.
- W249848954 modified "2023-09-23" @default.
- W249848954 title "Emplacement Scenarios for Volcanic Domes on Venus" @default.
- W249848954 hasPublicationYear "2012" @default.
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