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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>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7324</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-10-2965-2010</article-id>
<title-group>
<article-title>Uptake of NO&lt;sub&gt;3&lt;/sub&gt; and N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; to Saharan dust, ambient urban aerosol and soot: a relative rate study</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Tang</surname>
<given-names>M. J.</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>Thieser</surname>
<given-names>J.</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>Schuster</surname>
<given-names>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>Crowley</surname>
<given-names>J. N.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Max-Planck-Institute für Chemie, Atmospheric Chemistry Division, Mainz, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>29</day>
<month>03</month>
<year>2010</year>
</pub-date>
<volume>10</volume>
<issue>6</issue>
<fpage>2965</fpage>
<lpage>2974</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2010 M. J. Tang et al.</copyright-statement>
<copyright-year>2010</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://acp.copernicus.org/articles/10/2965/2010/acp-10-2965-2010.html">This article is available from https://acp.copernicus.org/articles/10/2965/2010/acp-10-2965-2010.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/articles/10/2965/2010/acp-10-2965-2010.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/10/2965/2010/acp-10-2965-2010.pdf</self-uri>
<abstract>
<p>The uptake of NO&lt;sub&gt;3&lt;/sub&gt; and N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; to Saharan dust, ambient aerosols
and soot was investigated using a novel and simple relative rate method with
simultaneous detection of both NO&lt;sub&gt;3&lt;/sub&gt; and N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt;. The use of
cavity ring down spectroscopy to detect both trace gases enabled the
measurements to be carried out at low mixing ratios (&amp;lt;500 pptv or 1&amp;times;10&lt;sup&gt;10&lt;/sup&gt; molecule cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt;). The uptake coefficient ratio,
&amp;gamma;(NO&lt;sub&gt;3&lt;/sub&gt;)/&amp;gamma;(N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt;), was determined to be 0.9&amp;plusmn;0.4 for Saharan dust, independent of relative humidity, NO&lt;sub&gt;3&lt;/sub&gt; or
N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; mixing ratio and exposure time. Ambient (urban) aerosols
showed a very limited capacity to take up N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; but were reactive
towards NO&lt;sub&gt;3&lt;/sub&gt; with &amp;gamma;(NO&lt;sub&gt;3&lt;/sub&gt;)/&amp;gamma;(N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt;)&gt;15.
A value of &amp;gamma;(NO&lt;sub&gt;3&lt;/sub&gt;)/&amp;gamma;(N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt;)~1.5–3 was obtained when using candle generated soot. The relative rate obtained
for Saharan dust can be placed on an absolute basis using our recently
determined value of &amp;gamma;(N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt;)=1&amp;times;10&lt;sup&gt;&amp;minus;2&lt;/sup&gt; to
give &amp;gamma;(NO&lt;sub&gt;3&lt;/sub&gt;)=9&amp;times;10&lt;sup&gt;&amp;minus;3&lt;/sup&gt;, which is significantly
smaller than the single previous value. With the present uptake coefficient,
reaction of NO&lt;sub&gt;3&lt;/sub&gt; with mineral dust will generally not contribute
significantly to its NO&lt;sub&gt;3&lt;/sub&gt; loss in the boundary atmosphere or to the
nitration of mineral dust.</p>
</abstract>
<counts><page-count count="10"/></counts>
</article-meta>
</front>
<body/>
<back>
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