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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-11-10433-2011</article-id>
<title-group>
<article-title>Quantification of the unknown HONO daytime source and its relation to NO&lt;sub&gt;2&lt;/sub&gt;</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sörgel</surname>
<given-names>M.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Regelin</surname>
<given-names>E.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Bozem</surname>
<given-names>H.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Diesch</surname>
<given-names>J.-M.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Drewnick</surname>
<given-names>F.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Fischer</surname>
<given-names>H.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Harder</surname>
<given-names>H.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Held</surname>
<given-names>A.</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>Hosaynali-Beygi</surname>
<given-names>Z.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Martinez</surname>
<given-names>M.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Zetzsch</surname>
<given-names>C.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>University of Bayreuth, Atmospheric Chemistry Research Laboratory, Bayreuth, Germany</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>University of Bayreuth, Junior Professorship in Atmospheric Chemistry, Bayreuth, Germany</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Max Planck Institute for Chemistry, Atmospheric Chemistry Department, P.O. Box 3060, 55020 Mainz, Germany</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Max Planck Institute for Chemistry, Particle Chemistry Department, P.O. Box 3060, 55020 Mainz, Germany</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Fraunhofer Institute for Toxicology and Experimental Medicine, Hannover, Germany</addr-line>
</aff>
<aff id="aff6">
<label>6</label>
<addr-line>now at: University Mainz, Institute for Atmospheric Physics, Mainz, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>20</day>
<month>10</month>
<year>2011</year>
</pub-date>
<volume>11</volume>
<issue>20</issue>
<fpage>10433</fpage>
<lpage>10447</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/11/10433/2011/acp-11-10433-2011.html">This article is available from http://www.atmos-chem-phys.net/11/10433/2011/acp-11-10433-2011.html</self-uri>
<self-uri xlink:href="http://www.atmos-chem-phys.net/11/10433/2011/acp-11-10433-2011.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/11/10433/2011/acp-11-10433-2011.pdf</self-uri>
<abstract>
<p>During the DOMINO (&lt;b&gt;D&lt;/b&gt;iel &lt;b&gt;O&lt;/b&gt;xidant &lt;b&gt;M&lt;/b&gt;echanism
&lt;b&gt;I&lt;/b&gt;n relation to &lt;b&gt;N&lt;/b&gt;itrogen &lt;b&gt;O&lt;/b&gt;xides) campaign in
southwest Spain we measured simultaneously all quantities necessary to
calculate a photostationary state for HONO in the gas phase. These
quantities comprise the concentrations of OH, NO, and HONO and the
photolysis frequency of NO&lt;sub&gt;2&lt;/sub&gt;, &lt;i&gt;j&lt;/i&gt;(NO&lt;sub&gt;2&lt;/sub&gt;) as a proxy for &lt;i&gt;j&lt;/i&gt;(HONO). This
allowed us to calculate values of the unknown HONO daytime source. This
unknown HONO source, normalized by NO&lt;sub&gt;2&lt;/sub&gt; mixing ratios and expressed as a
conversion frequency (% h&lt;sup&gt;&amp;minus;1&lt;/sup&gt;), showed a clear dependence on
&lt;i&gt;j&lt;/i&gt;(NO&lt;sub&gt;2&lt;/sub&gt;) with values up to 43% h&lt;sup&gt;−1&lt;/sup&gt; at noon. We compared our
unknown HONO source with values calculated from the measured field data for
two recently proposed processes, the light-induced NO&lt;sub&gt;2&lt;/sub&gt; conversion on
soot surfaces and the reaction of electronically excited NO&lt;sub&gt;2&lt;/sub&gt;* with
water vapour, with the result that these two reactions normally contributed
less than 10% (&lt;1% NO&lt;sub&gt;2&lt;/sub&gt; + soot + &lt;i&gt;h&lt;/i&gt;&amp;nu;; and &lt;10%
NO&lt;sub&gt;2&lt;/sub&gt;* + H&lt;sub&gt;2&lt;/sub&gt;O) to our unknown HONO daytime source. OH production from
HONO photolysis was found to be larger (by 20%) than the &quot;classical&quot;
OH formation from ozone photolysis (O(&lt;sup&gt;1&lt;/sup&gt;D)) integrated over the day.</p>
</abstract>
<counts><page-count count="15"/></counts>
</article-meta>
</front>
<body/>
<back>
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