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<article language="en">
	<journal>
		<journal_title>Atmospheric Chemistry and Physics Discussions</journal_title>
		<journal_url>www.atmos-chem-phys-discuss.net</journal_url>
		<issn>1680-7367</issn>
		<eissn>1680-7375</eissn>
		<volume_number>6</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acpd-6-7869-2006</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/6/7869/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/6/7869/2006/acpd-6-7869-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/6/7869/2006/acpd-6-7869-2006.pdf</fulltext_pdf>
	<start_page>7869</start_page>
	<end_page>7904</end_page>
	<publication_date>2006-08-14</publication_date>
	<article_title content_type="html">Investigations of the photochemical isotope equilibrium between O&lt;sub&gt;2&lt;/sub&gt;, CO&lt;sub&gt;2&lt;/sub&gt; and O&lt;sub&gt;3&lt;/sub&gt;</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>R. Shaheen</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>C. Janssen</name>
		</author>
		<author numeration="3" affiliations="1,2">
			<name>T. Röckmann</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Max-Planck-Institute for Nuclear Physics, Division of Atmospheric Physics, 69117 Heidelberg, Germany</affiliation>
		<affiliation numeration="2" content_type="html">Institute for Marine and Atmospheric Research Utrecht, Utrecht University, The Netherlands</affiliation>
	</affiliations>
	<abstract content_type="html">Contrary to tropospheric CO&lt;sub&gt;2&lt;/sub&gt; whose oxygen isotopic composition follows a
standard mass dependent relationship, i.e.&amp;nbsp;&amp;delta;&lt;sup&gt;17&lt;/sup&gt;O~0.5
&amp;delta;&lt;sup&gt;18&lt;/sup&gt;O, stratospheric CO&lt;sub&gt;2&lt;/sub&gt; is preferentially enriched in &lt;sup&gt;17&lt;/sup&gt;O,
leading to a strikingly different relation with &amp;delta;&lt;sup&gt;17&lt;/sup&gt;O~1.7&amp;delta;&lt;sup&gt;18&lt;/sup&gt;O. The isotope anomaly is likely inherited from O&lt;sub&gt;3&lt;/sub&gt; via photolytically produced O(&lt;sup&gt;1&lt;/sup&gt;D) that
undergoes isotope exchange with CO&lt;sub&gt;2&lt;/sub&gt; and the anomaly may well serve as a
tracer of stratospheric chemistry if details of the exchange mechanism are
understood. We have studied the photochemical isotope equilibrium in
UV-irradiated O&lt;sub&gt;2&lt;/sub&gt;-CO&lt;sub&gt;2&lt;/sub&gt; and O&lt;sub&gt;3&lt;/sub&gt;-CO&lt;sub&gt;2&lt;/sub&gt; mixtures to quantify the
transfer of the anomaly from O&lt;sub&gt;3&lt;/sub&gt; to CO&lt;sub&gt;2&lt;/sub&gt; at room temperature. By
following the time evolution of the oxygen isotopic compositions of CO&lt;sub&gt;2&lt;/sub&gt;
and O&lt;sub&gt;2&lt;/sub&gt; under varying initial isotopic compositions of both, O&lt;sub&gt;2&lt;/sub&gt;/O&lt;sub&gt;3&lt;/sub&gt;
and CO&lt;sub&gt;2&lt;/sub&gt;, the isotope equilibria between the two reservoirs were
determined. A very strong dependence of the isotope equilibrium on the
O&lt;sub&gt;2&lt;/sub&gt;/CO&lt;sub&gt;2&lt;/sub&gt;-ratio was established. Equilibrium enrichments of &lt;sup&gt;17&lt;/sup&gt;O and
&lt;sup&gt;18&lt;/sup&gt;O in CO&lt;sub&gt;2&lt;/sub&gt; relative to O&lt;sub&gt;2&lt;/sub&gt; diminish with increasing CO&lt;sub&gt;2&lt;/sub&gt; content,
and this reduction in the equilibrium enrichments does not follow a standard
mass dependent relation. When molecular oxygen exceeds the amount of CO&lt;sub&gt;2&lt;/sub&gt; by
a factor of about 20, &lt;sup&gt;17&lt;/sup&gt;O and &lt;sup&gt;18&lt;/sup&gt;O in equilibrated CO&lt;sub&gt;2&lt;/sub&gt; are enriched by
(142&amp;plusmn;4) and (146&amp;plusmn;4), respectively, at room
temperature and at a pressure of 225 hPa, independent of the
initial isotopic compositions of CO&lt;sub&gt;2&lt;/sub&gt; and O&lt;sub&gt;2&lt;/sub&gt; or O&lt;sub&gt;3&lt;/sub&gt;. From these
findings we derive a simple and general relation between the starting
isotopic compositions and amounts of O&lt;sub&gt;2&lt;/sub&gt; and CO&lt;sub&gt;2&lt;/sub&gt; and the observed
slope in a three oxygen isotope diagram. Predictions from this relation are
compared with published laboratory and atmospheric data.</abstract>
	<references>
	</references>
</article>

