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- W2000879224 abstract "We investigate the possibility of measuring the heights and morphology of viscously emplaced domes using radar imagery. We accurately reproduce the known height and shape of a terrestrial salt dome, and estimate the heights of several venusian pancake domes to within a factor of two. The terrestrial salt dome is consistent with a Bingham flow, while the much larger venusian pancake domes are consistent with a Newtonian flow. Applying the same techniques to Ganesa Macula, a potential cryovolcanic dome on Titan, we estimate a height between 2.0–4.9 km. Additional factors such as variable roughness and composition might account for some of the discrepancies observed." @default.
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- W2000879224 date "2008-08-01" @default.
- W2000879224 modified "2023-10-18" @default.
- W2000879224 title "Radar topography of domes on planetary surfaces" @default.
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- W2000879224 doi "https://doi.org/10.1016/j.icarus.2008.03.013" @default.
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