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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ACPD</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics Discussions</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACPD</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7375</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/acpd-12-11079-2012</article-id>
<title-group>
<article-title>Emissions of mercury in Southern Africa derived from long-term observations at Cape Point, South Africa</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Brunke</surname>
<given-names>E.-G.</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>Ebinghaus</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>Kock</surname>
<given-names>H. H.</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>Labuschagne</surname>
<given-names>C.</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="aff3">
<sup>3</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>South African Weather Service c/o CSIR, P.O. Box 320, Stellenbosch 7599, South Africa</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Helmholtz-Zentrum Geesthacht, Institute of Coastal Research, Max-Planck-Strasse, 21502 Geesthacht, Germany</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Max-Planck-Institut für Chemie, P.O. Box 3060, 55020 Mainz, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>02</day>
<month>05</month>
<year>2012</year>
</pub-date>
<volume>12</volume>
<issue>5</issue>
<fpage>11079</fpage>
<lpage>11103</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>Mercury emissions in South Africa have so far been estimated only by
  a bottom-up approach from activities and emission factors for
  different processes. In this paper we derive GEM/CO (GEM being
  gaseous elemental mercury, Hg&lt;sup&gt;0&lt;/sup&gt;), GEM/CO&lt;sub&gt;2&lt;/sub&gt;,
  GEM/CH&lt;sub&gt;4&lt;/sub&gt;, CO/CO&lt;sub&gt;2&lt;/sub&gt;, CH&lt;sub&gt;4&lt;/sub&gt;/CO&lt;sub&gt;2&lt;/sub&gt;, and
  CH&lt;sub&gt;4&lt;/sub&gt;/CO emission ratios from plumes observed during long-term
  monitoring of these species at Cape Point between March 2007 and
  December 2009. The average observed GEM/CO, GEM/CO&lt;sub&gt;2&lt;/sub&gt;,
  GEM/CH&lt;sub&gt;4&lt;/sub&gt;, CO/CO&lt;sub&gt;2&lt;/sub&gt;, CH&lt;sub&gt;4&lt;/sub&gt;/CO&lt;sub&gt;2&lt;/sub&gt;, and CH&lt;sub&gt;4&lt;/sub&gt;/CO
  emission ratios were 2.40 &amp;plusmn; 2.65 pg m&lt;sup&gt;&amp;minus;3&lt;/sup&gt; ppb&lt;sup&gt;&amp;minus;1&lt;/sup&gt;
  (&lt;i&gt;n&lt;/i&gt; = 47), 62.7 &amp;plusmn; 80.2 pg m&lt;sup&gt;&amp;minus;3&lt;/sup&gt; ppb&lt;sup&gt;&amp;minus;1&lt;/sup&gt; (&lt;i&gt;n&lt;/i&gt; = 44),
  3.61 &amp;plusmn; 4.66 pg m&lt;sup&gt;&amp;minus;3&lt;/sup&gt; ppb&lt;sup&gt;&amp;minus;1&lt;/sup&gt; (&lt;i&gt;n&lt;/i&gt; = 46), 35.6 &amp;plusmn;
  25.4 ppb ppm&lt;sup&gt;&amp;minus;1&lt;/sup&gt; (&lt;i&gt;n&lt;/i&gt; = 52), 20.2 &amp;plusmn;
  15.5 ppb ppm&lt;sup&gt;&amp;minus;1&lt;/sup&gt; (&lt;i&gt;n&lt;/i&gt;=48), and 0.876 &amp;plusmn;
  1.106 ppb ppm&lt;sup&gt;&amp;minus;1&lt;/sup&gt; (&lt;i&gt;n&lt;/i&gt;=42), respectively. The observed
  CO/CO&lt;sub&gt;2&lt;/sub&gt;, CH&lt;sub&gt;4&lt;/sub&gt;/CO&lt;sub&gt;2&lt;/sub&gt;, and CH&lt;sub&gt;4&lt;/sub&gt;/CO emission
  ratios agree within the combined uncertainties of the observations
  and emissions with the ratios calculated from EDGAR (version 4.2)
  CO&lt;sub&gt;2&lt;/sub&gt;, CO, and CH&lt;sub&gt;4&lt;/sub&gt; inventories for South Africa and
  Southern Africa (South Africa, Lesotho, Swaziland, Namibia,
  Botswana, Zimbabwe, and Mozambique) in 2007 and 2008 (inventories
  for 2009 are not available yet). Total elemental mercury emission of
  13.1, 15.2, and 16.1 t Hg yr&lt;sup&gt;&amp;minus;1&lt;/sup&gt; are estimated
  independently using the GEM/CO, GEM/CO&lt;sub&gt;2&lt;/sub&gt;, and GEM/CH&lt;sub&gt;4&lt;/sub&gt;
  emission ratios and the annual mean CO, CO&lt;sub&gt;2&lt;/sub&gt;, and CH&lt;sub&gt;4&lt;/sub&gt;
  emissions, respectively, of South Africa in 2007 and 2008. The
  average of these independent estimates of 14.8 &amp;plusmn;
  1.5 t GEM yr&lt;sup&gt;&amp;minus;1&lt;/sup&gt; is much less than the total emission of
  257 t Hg yr&lt;sup&gt;&amp;minus;1&lt;/sup&gt; from older inventories. Considering that
  emission of GEM represents only 50–78% of all mercury
  emissions, our estimates come close to the total mercury emission
  estimates ranging between 40–50 t Hg yr&lt;sup&gt;&amp;minus;1&lt;/sup&gt; from more
  recent inventories.</p>
</abstract>
<counts><page-count count="25"/></counts>
</article-meta>
</front>
<body/>
<back>
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