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	<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>9</volume_number>
		<issue_number>3</issue_number>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/acpd-9-13355-2009</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/9/13355/2009/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/9/13355/2009/acpd-9-13355-2009.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/9/13355/2009/acpd-9-13355-2009.pdf</fulltext_pdf>
	<start_page>13355</start_page>
	<end_page>13406</end_page>
	<publication_date>2009-06-17</publication_date>
	<article_title content_type="html">A photochemical model and sensitivity study of the triple-oxygen isotopic (&amp;Delta;&lt;sup&gt;17&lt;/sup&gt;O) composition of NO&lt;sub&gt;y&lt;/sub&gt;, HO&lt;sub&gt;x&lt;/sub&gt;, and H&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt; in a polluted boundary layer</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>G. Dominguez</name>
			<email>gdominguez@ucsd.edu</email>
		</author>
		<author numeration="2" affiliations="1,2">
			<name>G. Wilkins</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>M. H. Thiemens</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">University of California, San Diego, Department of Chemistry and Biochemistry, La Jolla, California, USA</affiliation>
		<affiliation numeration="2" content_type="html">University of California, Berkeley, Department of Mathematics, Berkeley, California, USA</affiliation>
	</affiliations>
	<abstract content_type="html">We present a photochemical model developed for the &lt;i&gt;explicit&lt;/i&gt;
calculation of triple oxygen isotopic compositions (&amp;Delta;&lt;sup&gt;17&lt;/sup&gt;O) of major
atmospheric species. While we focus on the  &amp;Delta;&lt;sup&gt;17&lt;/sup&gt;O of HNO&lt;sub&gt;3&lt;/sub&gt; and
aerosol nitrate (NO&lt;sup&gt;&amp;minus;&lt;/sup&gt;&lt;sub&gt;3&lt;/sub&gt;) and its precursors such as NO, NO&lt;sub&gt;2&lt;/sub&gt; and
N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt;, the general implementation given here also provides
&amp;Delta;&lt;sup&gt;17&lt;/sup&gt;O predictions for other important atmospheric compounds such
as OH, H&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt;, and HO&lt;sub&gt;2&lt;/sub&gt;. Through the use of a
simple aerosol surface area model, we calculate the &amp;Delta;&lt;sup&gt;17&lt;/sup&gt;O
composition of aerosol nitrate produced as a function of aerosol size and
aerosol surface type. We explore the sensitivity of the &amp;Delta;&lt;sup&gt;17&lt;/sup&gt;O of
atmospheric species through a series of sensitivity studies and show that the
&amp;Delta;&lt;sup&gt;17&lt;/sup&gt;O of atmospheric compounds is affected to various degrees by
environmental factors such as temperature, relative humidity, ozone
concentration, NO&lt;sub&gt;x&lt;/sub&gt; flux, and total ozone column density. In addition,
we find that &amp;Delta;&lt;sup&gt;17&lt;/sup&gt;O of these species is sensitive to photochemical
conditions such as cloud albedo, latitude, and time of year. We compare the
&amp;Delta;&lt;sup&gt;17&lt;/sup&gt;O calculation outputs to previous methods and find significant
differences in the &amp;Delta;&lt;sup&gt;17&lt;/sup&gt;O of NO&lt;sub&gt;2&lt;/sub&gt;. We describe the origins of
these and suggest studies that may help to resolve these differences.</abstract>
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