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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>Philip Swartzendruber</dc:contributor>
  <dc:contributor>Eric Prestbo</dc:contributor>
  <dc:creator>Colleen A. Caldwell</dc:creator>
  <dc:date>2006</dc:date>
  <dc:description>&lt;p&gt;This research was initiated to characterize atmospheric deposition of reactive gaseous mercury (RGM), particulate mercury (HgP; &amp;lt;2.5 &amp;mu;m), and gaseous elemental mercury (Hg&lt;sup&gt;0&lt;/sup&gt;) in the arid lands of south central New Mexico. Two methods were field-tested to estimate dry deposition of three mercury species. A manual speciation sampling train consisting of a KCl-coated denuder, 2.5 &amp;mu;m quartz fiber filters, and gold-coated quartz traps and an ion-exchange membrane (as a passive surrogate surface) were deployed concurrently over 24-h intervals for an entire year. The mean 24-h atmospheric concentration for RGM was 6.8 pg m&lt;sup&gt;-3&lt;/sup&gt;&lt;span&gt;&amp;nbsp;with an estimated deposition of 0.10 ng m&lt;/span&gt;&lt;sup&gt;-2&lt;/sup&gt;&lt;span&gt;h&lt;/span&gt;&lt;sup&gt;-1&lt;/sup&gt;. The estimated deposition of mercury to the passive surrogate surface was much greater (4.0 ng m&lt;sup&gt;-2&lt;/sup&gt;&lt;span&gt;h&lt;/span&gt;&lt;sup&gt;-1&lt;/sup&gt;) but demonstrated a diurnal pattern with elevated deposition from late afternoon to late evening (1400&amp;minus;2200; 8.0 ng m&lt;sup&gt;-2&lt;/sup&gt;&lt;span&gt;h&lt;/span&gt;&lt;sup&gt;-1&lt;/sup&gt;) and lowest deposition during the night just prior to sunrise (2200&amp;minus;0600; 1.7 ng m&lt;sup&gt;-2&lt;/sup&gt;h&lt;sup&gt;-1&lt;/sup&gt;). The mean 24-h atmospheric concentrations for HgP and Hg&lt;sup&gt;0&lt;/sup&gt;&lt;span&gt;&amp;nbsp;were 1.52 pg m&lt;/span&gt;&lt;sup&gt;-3&lt;/sup&gt;&lt;span&gt;&amp;nbsp;and 1.59 ng m&lt;/span&gt;&lt;sup&gt;-3&lt;/sup&gt;, respectively. Diurnal patterns were observed for RGM with atmospheric levels lowest during the night prior to sunrise (3.8 pg m-3) and greater during the afternoon and early evening (8.9 pg m&lt;sup&gt;-3&lt;/sup&gt;). Discernible diurnal patterns were not observed for either HgP or Hg&lt;sup&gt;0&lt;/sup&gt;. The total dry deposition of Hg was 5.9 &amp;mu;g m&lt;sup&gt;-2&lt;/sup&gt; year-1&lt;span&gt;&amp;nbsp;with the contribution from the three species as follows:&amp;thinsp; RGM (0.88 &amp;mu;g m&lt;/span&gt;&lt;sup&gt;-2&lt;/sup&gt;&lt;span&gt;&amp;nbsp;year&lt;/span&gt;&lt;sup&gt;-1&lt;/sup&gt;), HgP (0.025 &amp;mu;g m&lt;sup&gt;-2&lt;/sup&gt;&lt;span&gt;&amp;nbsp;year&lt;/span&gt;&lt;sup&gt;-1&lt;/sup&gt;), and Hg&lt;sup&gt;0&lt;/sup&gt;&lt;span&gt;&amp;nbsp;(5.0 &amp;mu;g m&lt;/span&gt;&lt;sup&gt;-2&lt;/sup&gt;&lt;span&gt;&amp;nbsp;year&lt;/span&gt;&lt;sup&gt;-1&lt;/sup&gt;). The annual wet deposition for total mercury throughout the same collection duration was 4.2 &amp;mu;g m&lt;sup&gt;-2&lt;/sup&gt;&lt;span&gt;&amp;nbsp;year&lt;/span&gt;&lt;sup&gt;-1&lt;/sup&gt;, resulting in an estimated total deposition of 10.1 &amp;mu;g m&lt;sup&gt;-2&lt;/sup&gt;&amp;nbsp;year&lt;sup&gt;-1&lt;/sup&gt;&lt;span&gt;&amp;nbsp;for Hg. On one sampling date, enhanced HgP (12 pg m&lt;/span&gt;&lt;sup&gt;-3&lt;/sup&gt;) was observed due to emissions from a wildfire approximately 250 km to the east.&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1021/es0609957</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>American Chemical Society</dc:publisher>
  <dc:title>Concentration and dry deposition of mercury species in arid south central New Mexico (2001-2002)</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>