<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>R. D. Lorenz</dc:contributor>
  <dc:contributor>R. L. Kirk</dc:contributor>
  <dc:creator>Catherine D. Neish</dc:creator>
  <dc:date>2008</dc:date>
  <dc:description>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. ?? 2008 Elsevier Inc.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1016/j.icarus.2008.03.013</dc:identifier>
  <dc:language>en</dc:language>
  <dc:title>Radar topography of domes on planetary surfaces</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>