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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>R. Pik</dc:contributor>
  <dc:contributor>J. Lave</dc:contributor>
  <dc:contributor>D. Bourles</dc:contributor>
  <dc:contributor>P.G. Burnard</dc:contributor>
  <dc:contributor>R. Yokochi</dc:contributor>
  <dc:contributor>B. Marty</dc:contributor>
  <dc:contributor>F. Trusdell</dc:contributor>
  <dc:creator>P.-H. Blard</dc:creator>
  <dc:date>2006</dc:date>
  <dc:description>&lt;div class="abstract svAbstract " data-etype="ab"&gt;&lt;p id=""&gt;Measurements of the cosmogenic &lt;sup&gt;3&lt;/sup&gt;He (&lt;sup&gt;3&lt;/sup&gt;He&lt;sub&gt;c&lt;/sub&gt;) content of various size aliquots of exposed olivines show that the fine fraction (&amp;lt;140&amp;nbsp;μm) has &lt;sup&gt;3&lt;/sup&gt;He&lt;sub&gt;c&lt;/sub&gt; concentrations between 14 and 100% lower than that of the coarse fractions (0.14–1&amp;nbsp;mm). Such differences attest to a grain size dependent partial release of &lt;sup&gt;3&lt;/sup&gt;He&lt;sub&gt;c&lt;/sub&gt; from the phenocrysts matrix during the preliminary in vacuo crushing. This result might have important implications since most&amp;nbsp;&lt;sup&gt;3&lt;/sup&gt;He&lt;sub&gt;c&lt;/sub&gt; measurements have used for ∼20&amp;nbsp;yr a standard routine based on the fusion of bulk&amp;nbsp;&lt;i&gt;powdered&lt;/i&gt; phenocrysts, whatever their grain size. A suite of new data obtained from coarse olivine grains yielded a mean Sea Level High Latitude &lt;sup&gt;3&lt;/sup&gt;He&lt;sub&gt;c&lt;/sub&gt; production rate (SLHL P&lt;sub&gt;3&lt;/sub&gt;) of 128±5 and 136±6&amp;nbsp;at. g&lt;sup&gt;−1&lt;/sup&gt; yr&lt;sup&gt;−1&lt;/sup&gt;, depending on the scaling factors used. This new value, which is ∼15% higher than previously published rates, is obtained from 5 ropy flow surfaces of Mt Etna (38°N) and Hawaiian (19°N) volcanoes, at elevations between sea level and 870&amp;nbsp;m and ranging in age from 1.47±0.05 to 149±23&amp;nbsp;ka according to independent &lt;sup&gt;14&lt;/sup&gt;C or K/Ar dating. &lt;sup&gt;3&lt;/sup&gt;He loss during the crushing step might account for the discrepancy between the standard reference value of 110–115&amp;nbsp;at. g&lt;sup&gt;−1&lt;/sup&gt; y&lt;sup&gt;−1&lt;/sup&gt; and the higher SLHL P&lt;sub&gt;3&lt;/sub&gt; proposed here. More generally, removal of the powdered fraction before fusion is an important point to consider in further studies in order to avoid any &lt;sup&gt;3&lt;/sup&gt;He&lt;sub&gt;c&amp;nbsp;&lt;/sub&gt;systematic underestimates.&lt;/p&gt;&lt;p id=""&gt;An altitudinal section has also been sampled on the ropy surface of a ∼1500&amp;nbsp;yr single flow of Mauna Loa (19°N) which allowed a new empirical atmospheric attenuation length of 149±22&amp;nbsp;g cm&lt;sup&gt;−2&lt;/sup&gt; to be documented for &lt;sup&gt;3&lt;/sup&gt;He&lt;sub&gt;c&lt;/sub&gt; in olivines between 2400 and 4000&amp;nbsp;m elevations.&lt;/p&gt;&lt;/div&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1016/j.epsl.2006.05.012</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>Elsevier</dc:publisher>
  <dc:title>Cosmogenic 3He production rates revisited from evidences of grain size dependent release of matrix-sited helium</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>