<?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>Frank T. Manheim</dc:contributor>
  <dc:contributor>J. M. Gieskes</dc:contributor>
  <dc:creator>P. C. Mangelsdorf Jr.</dc:creator>
  <dc:date>1970</dc:date>
  <dc:description>&lt;p&gt;Calculations show that gravitational settling of ions in an isothermal sediment column could produce increases of equilibrium concentrations in pore waters ranging from 1 percent per 100 m depth for chloride to 4 percent per 100 m depth for strontium.&lt;/p&gt;&lt;p&gt;The migration of ions in a thermal gradient (Soret effect) would cause minor salt enrichment upward toward the colder pole, but the presence of cation-exchanging particles such as clays would reverse this tendency and cause pumping of salt downward. A model calculation using literature data for the thermal potentials suggests that about 5-percent enrichment in Cl per 100 m depth may occur under steady-state conditions.&lt;/p&gt;&lt;p&gt;These mechanisms do not explain the greater enrichments commonly found in subsurface brines, but may modify salt distributions due to other phenomena.&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1306/5D25CA1B-16C1-11D7-8645000102C1865D</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>American Association of Petroleum Geologists</dc:publisher>
  <dc:title>Role of gravity, temperature gradients, and ion exchange media in the formation of fossil brines</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>