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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-8-1353-2008</article-id>
<title-group>
<article-title>Hydrogen isotope fractionation in the photolysis of formaldehyde</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Rhee</surname>
<given-names>T. S.</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>Brenninkmeijer</surname>
<given-names>C. A. M.</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>Röckmann</surname>
<given-names>T.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Korea Polar Research Institute, Incheon, Korea</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Atmospheric Chemistry Division, Max Planck Institute for Chemistry, Mainz, Germany</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Institute for Marine and Atmospheric Research Utrecht, Utrecht University, Utrecht, The Netherlands</addr-line>
</aff>
<pub-date pub-type="epub">
<day>07</day>
<month>03</month>
<year>2008</year>
</pub-date>
<volume>8</volume>
<issue>5</issue>
<fpage>1353</fpage>
<lpage>1366</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2008 T. S. Rhee et al.</copyright-statement>
<copyright-year>2008</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>
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<abstract>
<p>Experiments investigating the isotopic fractionation in the formation of
H&lt;sub&gt;2&lt;/sub&gt; by the photolysis of CH&lt;sub&gt;2&lt;/sub&gt;O under tropospheric conditions are
reported and discussed. The deuterium (D) depletion in the H&lt;sub&gt;2&lt;/sub&gt; produced
is 500(&amp;plusmn;20)&amp;permil; with respect to the parent CH&lt;sub&gt;2&lt;/sub&gt;O. We also observed
that complete photolysis of CH&lt;sub&gt;2&lt;/sub&gt;O under atmospheric conditions produces
H&lt;sub&gt;2&lt;/sub&gt; that has virtually the same isotope ratio as that of the parent
CH&lt;sub&gt;2&lt;/sub&gt;O. These findings imply that there must be a very strong concomitant
isotopic enrichment in the radical channel (CH&lt;sub&gt;2&lt;/sub&gt;O+&lt;i&gt;h&lt;/i&gt;&amp;nu; &amp;rarr; CHO+H) as
compared to the molecular channel (CH&lt;sub&gt;2&lt;/sub&gt;O+&lt;i&gt;h&lt;/i&gt;&amp;nu; &amp;rarr; H&lt;sub&gt;2&lt;/sub&gt;+CO) of the
photolysis of CH&lt;sub&gt;2&lt;/sub&gt;O in order to balance the relatively small isotopic
fractionation in the competing reaction of CH&lt;sub&gt;2&lt;/sub&gt;O with OH. Using a 1-box
photochemistry model we calculated the isotopic fractionation factor for the
radical channel to be 0.22(&amp;plusmn;0.08), which is equivalent to a 780(&amp;plusmn;80)&amp;permil;
enrichment in D of the remaining CH&lt;sub&gt;2&lt;/sub&gt;O. When CH&lt;sub&gt;2&lt;/sub&gt;O is in
photochemical steady state, the isotope ratio of the H&lt;sub&gt;2&lt;/sub&gt; produced is
determined not only by the isotopic fractionation occurring during the
photolytical production of H&lt;sub&gt;2&lt;/sub&gt; (&amp;alpha;&lt;sub&gt;&lt;i&gt;m&lt;/i&gt;&lt;/sub&gt;) but also by overall
fractionation for the removal processes of CH&lt;sub&gt;2&lt;/sub&gt;O (&amp;alpha;&lt;sub&gt;&lt;i&gt;f&lt;/i&gt;&lt;/sub&gt;), and is
represented by the ratio of &amp;alpha;&lt;sub&gt;&lt;i&gt;m&lt;/i&gt;&lt;/sub&gt;/&amp;alpha;&lt;sub&gt;&lt;i&gt;f&lt;/i&gt;&lt;/sub&gt;. Applying the isotopic
fractionation factors relevant to CH&lt;sub&gt;2&lt;/sub&gt;O photolysis obtained in the
present study to the troposphere, the ratio of &amp;alpha;&lt;sub&gt;&lt;i&gt;m&lt;/i&gt;&lt;/sub&gt;/&amp;alpha;&lt;sub&gt;&lt;i&gt;f&lt;/i&gt;&lt;/sub&gt; varies from
~0.8 to ~1.2 depending on the fraction of CH&lt;sub&gt;2&lt;/sub&gt;O that reacts
with OH and that produces H&lt;sub&gt;2&lt;/sub&gt;. This range of &amp;alpha;&lt;sub&gt;&lt;i&gt;m&lt;/i&gt;&lt;/sub&gt;/&amp;alpha;&lt;sub&gt;&lt;i&gt;f&lt;/i&gt;&lt;/sub&gt; can render
the H&lt;sub&gt;2&lt;/sub&gt; produced from the photochemical oxidation of CH&lt;sub&gt;4&lt;/sub&gt; to be
enriched in D (with respect to the original CH&lt;sub&gt;4&lt;/sub&gt;) by the factor of 1.2&amp;ndash;1.3 as anticipated in the literature.</p>
</abstract>
<counts><page-count count="14"/></counts>
</article-meta>
</front>
<body/>
<back>
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