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<journal-meta>
<journal-id journal-id-type="publisher">ACP</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7324</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-3-535-2003</article-id>
<title-group>
<article-title>A numerical modelling study on regional mercury budget for eastern North America</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Lin</surname>
<given-names>X.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Tao</surname>
<given-names>Y.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Kinectrics, 800 Kipling Avenue, Toronto, M8Z 6C4, Canada</addr-line>
</aff>
<pub-date pub-type="epub">
<day>26</day>
<month>05</month>
<year>2003</year>
</pub-date>
<volume>3</volume>
<issue>3</issue>
<fpage>535</fpage>
<lpage>548</lpage>
<permissions>
<license xlink:type="simple">
<license-p>This is an open-access article ditributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.</license-p>
</license>
</permissions>
<self-uri xlink:href="http://www.atmos-chem-phys.net/3/535/2003/acp-3-535-2003.html">This article is available from http://www.atmos-chem-phys.net/3/535/2003/acp-3-535-2003.html</self-uri>
<self-uri xlink:href="http://www.atmos-chem-phys.net/3/535/2003/acp-3-535-2003.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/3/535/2003/acp-3-535-2003.pdf</self-uri>
<abstract>
<p>In this study, we have integrated an up-to-date
      physio-chemical transformation mechanism of Hg into the framework of US EPA&apos;s CMAQ model system.  In addition, the
      model adapted detailed calculations of the air-surface exchange for Hg to properly
      describe Hg re-emissions and dry deposition from and to natural surfaces.  The
      mechanism covers Hg in three categories, elemental Hg (Hg&lt;sup&gt;0&lt;/sup&gt;), reactive gaseous Hg
      (RGM) and particulate Hg (HgP).  With interfacing to MM5 (meteorology processor) and
      SMOKE (emission processor), we applied the model to a 4-week period in June/July
      1995 on a domain covering most of eastern North America.  Results indicate that the
      model simulates reasonably well the levels of total gaseous Hg (TGM) and the specific
      Hg wet deposition measurements made by the Hg deposition network (MDN). Moreover, results from various scenario runs reveal that the Hg system behaves in a
      closely linear way in terms of contributions from different source categories, i.e.
      anthropogenic emissions, natural re-emissions and background.  Analyses of the
      scenario results suggest that 37% of anthropogenically emitted Hg was deposited back
      in the model domain with 5155 kg of anthropogenic Hg moving out of the domain during
      the simulation period.  Overall, the domain served as a net source, which supplied
      ~a half ton of Hg to the global background pool over the period.  Our model validation and a
      sensitivity test further rationalized the rate constant for gaseous oxidation of
      Hg&lt;sup&gt;0&lt;/sup&gt; by hydroxyl radical OH used in the global scale modelling study by Bergan and Rodhe
      (2001).  A further laboratory determination of the reaction rate constant, including its
      temperature dependence, stands as one of the important issues critical to improving our
      knowledge on the budget and cycling of Hg.</p>
</abstract>
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