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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>Richard F. Madole</dc:contributor>
  <dc:contributor>P. Kubik</dc:contributor>
  <dc:contributor>Richard R. McDonald</dc:contributor>
  <dc:creator>Larry Benson</dc:creator>
  <dc:date>2007</dc:date>
  <dc:description>&lt;p&gt;&lt;span&gt;Surface-exposure (&lt;/span&gt;&lt;sup&gt;10&lt;/sup&gt;&lt;span&gt;Be) ages have been obtained on boulders from three post-Pinedale&amp;nbsp;&lt;a title="Learn more about Glacial Drift from ScienceDirect's AI-generated Topic Pages" href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/glacial-drift" data-mce-href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/glacial-drift"&gt;end-moraine&lt;/a&gt;&amp;nbsp;complexes in the Front Range, Colorado. Boulder rounding appears related to the cirque-to-moraine transport distance at each site with subrounded boulders being typical of the 2-km-long Chicago Lakes Glacier, subangular boulders being typical of the 1-km-long Butler Gulch Glacier, and angular boulders being typical of the few-hundred-m-long Isabelle Glacier. Surface-exposure ages of angular boulders from the Isabelle Glacier moraine, which formed during the&amp;nbsp;&lt;a title="Learn more about Little Ice Age from ScienceDirect's AI-generated Topic Pages" href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/little-ice-age" data-mce-href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/little-ice-age"&gt;Little Ice Age&lt;/a&gt;&amp;nbsp;(LIA) according to previous lichenometric dating, indicate cosmogenic inheritance values ranging from 0 to ∼3.0&amp;nbsp;&lt;/span&gt;&lt;sup&gt;10&lt;/sup&gt;&lt;span&gt;Be&lt;/span&gt;&lt;span&gt;&amp;nbsp;&lt;/span&gt;&lt;span&gt;ka.&lt;/span&gt;&lt;a class="workspace-trigger" name="bfn1" href="https://www.sciencedirect.com/science/article/pii/S0277379107000650?via%3Dihub#fn1" data-mce-href="https://www.sciencedirect.com/science/article/pii/S0277379107000650?via%3Dihub#fn1"&gt;&lt;sup&gt;1&lt;/sup&gt;&lt;/a&gt;&lt;span&gt;&amp;nbsp;Subangular boulders from the Butler Gulch end moraine yielded surface-exposure ages ranging from 5 to 10.2&amp;nbsp;&lt;/span&gt;&lt;sup&gt;10&lt;/sup&gt;&lt;span&gt;Be&lt;/span&gt;&lt;span&gt;&amp;nbsp;&lt;/span&gt;&lt;span&gt;ka. We suggest that this moraine was deposited during the 8.2&lt;/span&gt;&lt;span&gt;&amp;nbsp;&lt;/span&gt;&lt;span&gt;cal&lt;/span&gt;&lt;span&gt;&amp;nbsp;&lt;/span&gt;&lt;span&gt;ka event, which has been associated with&amp;nbsp;&lt;a title="Learn more about Outburst from ScienceDirect's AI-generated Topic Pages" href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/outburst" data-mce-href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/outburst"&gt;outburst&lt;/a&gt;&amp;nbsp;floods from Lake Agassiz and Lake Ojibway, and that the large age range associated with the Butler Gulch end moraine is caused by cosmogenic shielding of and(or)&amp;nbsp;&lt;a title="Learn more about Spalling from ScienceDirect's AI-generated Topic Pages" href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/spalling" data-mce-href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/spalling"&gt;spalling&lt;/a&gt;&amp;nbsp;from boulders that have ages in the younger part of the range and by cosmogenic inheritance in boulders that have ages in the older part of the range. The surface-exposure ages of eight of nine subrounded boulders from the Chicago Lakes area fall within the 13.0–11.7&amp;nbsp;&lt;/span&gt;&lt;sup&gt;10&lt;/sup&gt;&lt;span&gt;Be&lt;/span&gt;&lt;span&gt;&amp;nbsp;&lt;/span&gt;&lt;span&gt;ka age range, and appear to have been deposited during the&amp;nbsp;&lt;a title="Learn more about Younger Dryas from ScienceDirect's AI-generated Topic Pages" href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/younger-dryas" data-mce-href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/younger-dryas"&gt;Younger Dryas&lt;/a&gt;&amp;nbsp;interval. The general lack of inheritance in the eight samples probably stems from the fact that only a few thousand years intervened between the retreat of the Pinedale glacier and the advance of the Chicago Lakes glacier; in addition,&amp;nbsp;&lt;a title="Learn more about Bedrock from ScienceDirect's AI-generated Topic Pages" href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/bedrock" data-mce-href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/bedrock"&gt;bedrock&lt;/a&gt;&amp;nbsp;in the Chicago Lakes&amp;nbsp;&lt;a title="Learn more about Cirque from ScienceDirect's AI-generated Topic Pages" href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/cirque" data-mce-href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/cirque"&gt;cirque&lt;/a&gt;&amp;nbsp;area may have remained covered with snow and ice during that interval, thus partially shielding the bedrock from cosmogenic radiation.&lt;/span&gt;&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1016/j.quascirev.2007.02.015</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>Elsevier</dc:publisher>
  <dc:title>Surface-exposure ages of Front Range moraines that may have formed during the Younger Dryas, 8.2 cal ka, and Little Ice Age events</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>