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<front>
<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-8-7165-2008</article-id>
<title-group>
<article-title>Simulation of atmospheric mercury depletion events (AMDEs) during  polar springtime using the MECCA box model</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Xie</surname>
<given-names>Z.-Q.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sander</surname>
<given-names>R.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Pöschl</surname>
<given-names>U.</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>Slemr</surname>
<given-names>F.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Biogeochemistry Department, Max Planck Institute for Chemistry, P.O. Box 3060, 55020 Mainz, Germany</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Air Chemistry Department, Max Planck Institute for Chemistry, P.O. Box 3060, 55020 Mainz, Germany</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>also at: Institute of Polar Environment, University of Science and Technology of China, Hefei, Anhui, 230026, P. R. China</addr-line>
</aff>
<pub-date pub-type="epub">
<day>09</day>
<month>12</month>
<year>2008</year>
</pub-date>
<volume>8</volume>
<issue>23</issue>
<fpage>7165</fpage>
<lpage>7180</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>
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<abstract>
<p>Atmospheric mercury depletion events (AMDEs) during polar springtime
  are closely correlated with bromine-catalyzed tropospheric ozone
  depletion events (ODEs). To study gas- and aqueous-phase reaction
  kinetics and speciation of mercury during AMDEs, we have included
  mercury chemistry into the box model MECCA (Module Efficiently
  Calculating the Chemistry of the Atmosphere), which enables dynamic
  simulation of bromine activation and ODEs.

&lt;br&gt;&lt;br&gt;

  We found that the reaction of Hg with Br atoms dominates the loss of
  gaseous elemental mercury (GEM). To explain the experimentally
  observed synchronous depletion of GEM and O&lt;sub&gt;3&lt;/sub&gt;, the reaction
  rate of Hg+BrO has to be much lower than that of Hg+Br. The
  synchronicity is best reproduced with rate coefficients at the lower
  limit of the literature values for both reactions, i.e.
  &lt;I&gt;k&lt;/I&gt;&lt;sub&gt;Hg+Br&lt;/sub&gt;&amp;asymp;3&amp;times;10&lt;sup&gt;&amp;minus;13&lt;/sup&gt; and &lt;I&gt;k&lt;/I&gt;&lt;sub&gt;Hg+BrO&lt;/sub&gt;&amp;le;1&amp;times;10&lt;sup&gt;&amp;minus;15&lt;/sup&gt; cm&lt;sup&gt;3&lt;/sup&gt; molecule&lt;sup&gt;&amp;minus;1&lt;/sup&gt; s&lt;sup&gt;&amp;minus;1&lt;/sup&gt;, respectively.

&lt;br&gt;&lt;br&gt;

  Throughout the simulated AMDEs, \chem{BrHgOBr} was the most abundant
  reactive mercury species, both in the gas phase and in the aqueous
  phase. The aqueous-phase concentrations of BrHgOBr,
  HgBr&lt;sub&gt;2&lt;/sub&gt;, and HgCl&lt;sub&gt;2&lt;/sub&gt; were several orders of magnitude
  larger than that of Hg(SO&lt;sub&gt;3&lt;/sub&gt;)&lt;sub&gt;2&lt;/sub&gt;&lt;sup&gt;2&amp;minus;&lt;/sup&gt;.

&lt;br&gt;&lt;br&gt;

  Considering chlorine chemistry outside depletion events (i.e. without
  bromine activation), the concentration of total divalent mercury in
  sea-salt aerosol particles (mostly HgCl&lt;sub&gt;4&lt;/sub&gt;&lt;sup&gt;2&amp;minus;&lt;/sup&gt;) was much higher than
  in dilute aqueous droplets (mostly Hg(SO&lt;sub&gt;3&lt;/sub&gt;)&lt;sub&gt;2&lt;/sub&gt;&lt;sup&gt;2&amp;minus;&lt;/sup&gt;), and did
  not exhibit a diurnal cycle (no correlation with HO&lt;sub&gt;2&lt;/sub&gt;
  radicals).</p>
</abstract>
<counts><page-count count="16"/></counts>
</article-meta>
</front>
<body/>
<back>
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