<?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>Colin M. Dundas</dc:contributor>
  <dc:contributor>Melinda A. Kahre</dc:contributor>
  <dc:creator>Kaj E. Williams</dc:creator>
  <dc:date>2022</dc:date>
  <dc:description>Mid-latitude exposed ice scarps have recently been identified on Mars (Dundas et al., 2018; 2021). The presence of such surface ice exposures at relatively low latitudes was itself a mystery, and the formation dynamics of such scarps have also not been explained. In this work we model the ice ablation rates of several identified mid-latitude scarps. We find that, given certain characteristics of their geographic setting, the orientation and growth of the scarps can be explained by energy balance models.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1016/j.icarus.2022.115174</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>Elsevier</dc:publisher>
  <dc:title>The formation mechanisms for mid-latitude ice scarps on Mars</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>