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<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd">
<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" article-type="research-article" dtd-version="3.0" xml:lang="en">
<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-1-1-2001</article-id>
<title-group>
<article-title>298 K rate coefficients for the reaction of OH with &lt;i&gt;i&lt;/i&gt; - C&lt;sub&gt;3&lt;/sub&gt;H&lt;sub&gt;7&lt;/sub&gt;I, &lt;i&gt;n&lt;/i&gt; - C&lt;sub&gt;3&lt;/sub&gt;H&lt;sub&gt;7&lt;/sub&gt;I and C&lt;sub&gt;3&lt;/sub&gt;H&lt;sub&gt;8&lt;/sub&gt;</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Carl</surname>
<given-names>S. A.</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="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Department of Chemistry, University of Leuven, Celestijnenlaan 200F, B-3001 Leuven, Belgium</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Max-Planck-Institut für Chemie, Division of Atmospheric Chemistry, Postfach 3060, D-55020 Mainz, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>22</day>
<month>11</month>
<year>2001</year>
</pub-date>
<volume>1</volume>
<issue>1</issue>
<fpage>1</fpage>
<lpage>7</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/1/1/2001/acp-1-1-2001.html">This article is available from http://www.atmos-chem-phys.net/1/1/2001/acp-1-1-2001.html</self-uri>
<self-uri xlink:href="http://www.atmos-chem-phys.net/1/1/2001/acp-1-1-2001.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/1/1/2001/acp-1-1-2001.pdf</self-uri>
<abstract>
<p>The kinetics of
the title reactions were investigated using the laser photolysis - resonance
fluorescence method, employing the sequential two-photon dissociation of NO&lt;sub&gt;2&lt;/sub&gt;
in the 
presence of H&lt;sub&gt;2&lt;/sub&gt;&amp;nbsp; as the OH source. The 298 K rate constant for OH
+ C&lt;sub&gt;3&lt;/sub&gt;H&lt;sub&gt;8&lt;/sub&gt; was found to be (1.15 ± 0.1) × 10&lt;sup&gt;-12&lt;/sup&gt;
cm&lt;sup&gt;3&lt;/sup&gt; s&lt;sup&gt;-1&lt;/sup&gt;, in excellent agreement with the literature
recommendation, and with a separate determination using HNO&lt;sub&gt;3&lt;/sub&gt;&amp;nbsp;
photolysis at 248 nm as the OH source. The 298 K rate constants for OH + &lt;i&gt;n
&lt;/i&gt;- C&lt;sub&gt;3&lt;/sub&gt;H&lt;sub&gt;7&lt;/sub&gt;I
and&amp;nbsp; &lt;i&gt;i &lt;/i&gt;-
C&lt;sub&gt;3&lt;/sub&gt;H&lt;sub&gt;7&lt;/sub&gt;I&amp;nbsp; were measured for the first time and found to
be (1.47 ± 0.08) and (1.22 ± 0.06) × 10&lt;sup&gt;-12&lt;/sup&gt; cm&lt;sup&gt;3&lt;/sup&gt;
s&lt;sup&gt;-1&lt;/sup&gt;, respectively. The errors include an assessment of systematic
error due to concentration measurement, which, for the propyl-iodides was
minimised by on-line UV-absorption spectroscopy. These results show that
reaction with OH is an important sink for&amp;nbsp;
&lt;i&gt;n &lt;/i&gt;-
C&lt;sub&gt;3&lt;/sub&gt;H&lt;sub&gt;7&lt;/sub&gt;I and&amp;nbsp;
&lt;i&gt;i &lt;/i&gt;-
C&lt;sub&gt;3&lt;/sub&gt;H&lt;sub&gt;7&lt;/sub&gt;I, which has implications for the reactive iodine
budget of the marine boundary layer.</p>
</abstract>
<counts><page-count count="7"/></counts>
</article-meta>
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