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<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>J. M. Williams</dc:contributor>
  <dc:contributor>R.B. Anderson</dc:contributor>
  <dc:contributor>L.A. Edgar</dc:contributor>
  <dc:contributor>H. Newsom</dc:contributor>
  <dc:contributor>S. Le Mouélic</dc:contributor>
  <dc:contributor>M. Minitti</dc:contributor>
  <dc:contributor>R. Wiens</dc:contributor>
  <dc:contributor>S. Maurice</dc:contributor>
  <dc:creator>A. J. Williams III</dc:creator>
  <dc:date>2014</dc:date>
  <dc:description>Analysis of grain size distribution from RMI mosaics (Curiosity) are used to better define variations in grain size and facies in the Shaler outcrop.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:language>en</dc:language>
  <dc:publisher>Lunar and Planetary Institute</dc:publisher>
  <dc:title>Determining grain characteristics in the Shaler Outcrop with ChemCam Remote Micro-Imager mosaics</dc:title>
  <dc:type>text</dc:type>
</oai_dc:dc>