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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-8-5033-2008</article-id>
<title-group>
<article-title>What can &lt;sup&gt;14&lt;/sup&gt;CO measurements tell us about OH?</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Krol</surname>
<given-names>M. C.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</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>Meirink</surname>
<given-names>J. F.</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>Bergamaschi</surname>
<given-names>P.</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>Mak</surname>
<given-names>J. E.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Lowe</surname>
<given-names>D.</given-names>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Jöckel</surname>
<given-names>P.</given-names>
</name>
<xref ref-type="aff" rid="aff7">
<sup>7</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Houweling</surname>
<given-names>S.</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>Röckmann</surname>
<given-names>T.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Netherlands Institute for Space Research (SRON), Utrecht, The Netherlands</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Institute for Marine and Atmospheric Research Utrecht (IMAU), Utrecht, The Netherlands</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Wageningen University and Research Centre (WUR), Wageningen, The Netherlands</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>European Commission Joint Research Centre, Institute for Environment and Sustainability, Ispra, Italy</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Institute for Terrestrial and Planetary Atmospheres, Stony Brook University, NY, USA</addr-line>
</aff>
<aff id="aff6">
<label>6</label>
<addr-line>National Institute of Water and Atmospheric Research, Wellington, New Zealand</addr-line>
</aff>
<aff id="aff7">
<label>7</label>
<addr-line>Max Planck Institute for Chemistry, Mainz, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>29</day>
<month>08</month>
<year>2008</year>
</pub-date>
<volume>8</volume>
<issue>16</issue>
<fpage>5033</fpage>
<lpage>5044</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>The possible use of &lt;sup&gt;14&lt;/sup&gt;CO measurements to constrain hydroxyl radical
(OH) concentrations in the atmosphere is investigated. &lt;sup&gt;14&lt;/sup&gt;CO is mainly
produced in the upper atmosphere from cosmic radiation. Measurements of
&lt;sup&gt;14&lt;/sup&gt;CO at the surface show lower concentrations compared to the upper
atmospheric source region, which is the result of oxidation by OH. In this
paper, the sensitivity of &lt;sup&gt;14&lt;/sup&gt;CO mixing ratio surface measurements to the
3-D OH distribution is assessed with the TM5 model. Simulated &lt;sup&gt;14&lt;/sup&gt;CO
mixing ratios agree within a few molecules &lt;sup&gt;14&lt;/sup&gt;CO cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt; (STP) with
existing measurements at five locations worldwide. The simulated cosmogenic
&lt;sup&gt;14&lt;/sup&gt;CO distribution appears mainly sensitive to the assumed upper
atmospheric &lt;sup&gt;14&lt;/sup&gt;C source function, and to a lesser extend to model
resolution. As a next step, the sensitivity of &lt;sup&gt;14&lt;/sup&gt;CO measurements to OH
is calculated with the adjoint TM5 model. The results indicate that
&lt;sup&gt;14&lt;/sup&gt;CO measurements taken in the tropics are sensitive to OH in a
spatially confined region that varies strongly over time due to
meteorological variability. Given measurements with an accuracy of 0.5 molecules &lt;sup&gt;14&lt;/sup&gt;CO cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt; STP,
a good characterization of the cosmogenic
&lt;sup&gt;14&lt;/sup&gt;CO fraction, and assuming perfect transport modeling, a single
&lt;sup&gt;14&lt;/sup&gt;CO measurement may constrain OH to 0.2–0.3&amp;times;10&lt;sup&gt;6&lt;/sup&gt; molecules OH cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt; on time scales of 6 months and spatial scales of
70&amp;times;70 degrees (latitude&amp;times;longitude) between the surface and
500 hPa. The sensitivity of &lt;sup&gt;14&lt;/sup&gt;CO measurements to high latitude OH is
about a factor of five higher. This is in contrast with methyl chloroform
(MCF) measurements, which show the highest sensitivity to tropical OH,
mainly due to the temperature dependent rate constant of the MCF–OH
reaction. A logical next step will be the analysis of existing &lt;sup&gt;14&lt;/sup&gt;CO
measurements in an inverse modeling framework. This paper presents the
required mathematical framework for such an analysis.</p>
</abstract>
<counts><page-count count="12"/></counts>
</article-meta>
</front>
<body/>
<back>
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