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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>T.-L. Ku</dc:contributor>
  <dc:contributor>J.D. Macdougall</dc:contributor>
  <dc:contributor>V.M. Burns</dc:contributor>
  <dc:contributor>R. Burns</dc:contributor>
  <dc:contributor>J. Dymond</dc:contributor>
  <dc:contributor>M.W. Lyle</dc:contributor>
  <dc:contributor>D.Z. Piper</dc:contributor>
  <dc:creator>W.S. Moore</dc:creator>
  <dc:date>1981</dc:date>
  <dc:description>&lt;div id="abstracts" class="Abstracts u-font-serif text-s"&gt;&lt;div id="ab1" class="abstract author" lang="en"&gt;&lt;div id="aep-abstract-sec-id9"&gt;&lt;p&gt;Fluxes of metals to the top and bottom surfaces of a manganese nodule were determined by combining radiochemical (&lt;sup&gt;230&lt;/sup&gt;Th,&lt;sup&gt;231&lt;/sup&gt;Pa,&lt;sup&gt;232&lt;/sup&gt;Th,&lt;sup&gt;238&lt;/sup&gt;U,&lt;sup&gt;234&lt;/sup&gt;U) and detailed chemical data. The top of the nodule had been growing in its collected orientation at 4.7 mm Myr&lt;sup&gt;−1&lt;/sup&gt;&lt;span&gt;&amp;nbsp;&lt;/span&gt;for at least 0.5 Myr and accreting Mn at 200 μg cm&lt;sup&gt;−2&lt;/sup&gt;&lt;span&gt;&amp;nbsp;&lt;/span&gt;kyr&lt;sup&gt;−1&lt;/sup&gt;. The bottom of the nodule had been growing in its collected orientation at about 12 mm Myr&lt;sup&gt;−1&lt;/sup&gt;&lt;span&gt;&amp;nbsp;&lt;/span&gt;for at least 0.3 Myr and accreting Mn at about 700 μg cm&lt;sup&gt;−2&lt;/sup&gt;&lt;span&gt;&amp;nbsp;&lt;/span&gt;yr&lt;sup&gt;−1&lt;/sup&gt;. Although the top of the nodule was enriched in iron relative to the bottom, the nodule had been accreting Fe 50% faster on the bottom.&lt;sup&gt;232&lt;/sup&gt;Th was also accumulating more rapidly in the bottom despite a 20-fold enrichment of&lt;sup&gt;230&lt;/sup&gt;Th on the top.&lt;/p&gt;&lt;p&gt;The distribution of alpha-emitting nuclides calculated from detailed radiochemical measurements matched closely the pattern revealed by 109-day exposures of alpha-sensitive film to the nodule. However, the shape and slope of the total alpha profile with depth into the nodule was affected strongly by&lt;sup&gt;226&lt;/sup&gt;Ra and&lt;sup&gt;222&lt;/sup&gt;Rn migrations making the alpha-track technique alone an inadequate method of measuring nodule growth rates.&lt;/p&gt;&lt;p&gt;Diffusion of radium in the nodule may have been affected by diagenetic reactions which produce barite, phillipsite and todorokite within 1 mm of the nodule surface; however, our sampling interval was too broad to document the effect. We have not been able to resolve the importance of nodule diagenesis on the gross chemistry of the nodule.&lt;/p&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1016/0012-821X(81)90217-X</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>Elsevier</dc:publisher>
  <dc:title>Fluxes of metals to a manganese nodule: Radiochemical, chemical, structural, and mineralogical studies</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>