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	<journal>
		<journal_title>Atmospheric Chemistry and Physics</journal_title>
		<journal_url>www.atmos-chem-phys.net</journal_url>
		<issn>1680-7316</issn>
		<eissn>1680-7324</eissn>
		<volume_number>8</volume_number>
		<issue_number>16</issue_number>
		<publication_year>2008</publication_year>
	</journal>
	<doi>10.5194/acp-8-4855-2008</doi>
	<article_url>http://www.atmos-chem-phys.net/8/4855/2008/</article_url>
	<abstract_html>http://www.atmos-chem-phys.net/8/4855/2008/acp-8-4855-2008.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys.net/8/4855/2008/acp-8-4855-2008.pdf</fulltext_pdf>
	<start_page>4855</start_page>
	<end_page>4864</end_page>
	<publication_date>2008-08-21</publication_date>
	<article_title content_type="html">Multiphase modeling of nitrate photochemistry in the quasi-liquid layer (QLL): implications for NO&lt;sub&gt;x&lt;/sub&gt; release from the Arctic and coastal Antarctic snowpack</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>C. S. Boxe</name>
			<email>christopher.boxe@jpl.nasa.gov</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>A. Saiz-Lopez</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Earth and Space Science Div., NASA Jet Propulsion Laboratory, California Inst. of Technology, Pasadena, CA 91109, USA</affiliation>
	</affiliations>
	<abstract content_type="html">We utilize a multiphase model, CON-AIR (&lt;B&gt;Con&lt;/B&gt;densed Phase to
&lt;B&gt;Air&lt;/B&gt; Transfer Model), to show that the photochemistry of nitrate
(NO&lt;sub&gt;3&lt;/sub&gt;&lt;sup&gt;&amp;minus;&lt;/sup&gt;) in and on ice and snow surfaces, specifically the
quasi-liquid layer (QLL), can account for NO&lt;sub&gt;x&lt;/sub&gt; volume fluxes,
concentrations, and [NO]/[NO&lt;sub&gt;2&lt;/sub&gt;] (γ=[NO]/[NO&lt;sub&gt;2&lt;/sub&gt;]) measured just above the Arctic and coastal
Antarctic snowpack. Maximum gas phase NO&lt;sub&gt;x&lt;/sub&gt; volume fluxes, concentrations
and γ simulated for spring and summer range from 5.0&amp;times;10&lt;sup&gt;4&lt;/sup&gt; to
6.4&amp;times;10&lt;sup&gt;5&lt;/sup&gt; molecules cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt; s&lt;sup&gt;&amp;minus;1&lt;/sup&gt;, 5.7&amp;times;10&lt;sup&gt;8&lt;/sup&gt; to 4.8&amp;times;10&lt;sup&gt;9&lt;/sup&gt; molecules cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt;,
and ~0.8 to 2.2, respectively, which are comparable to gas phase NO&lt;sub&gt;x&lt;/sub&gt;
volume fluxes, concentrations and γ measured in the field. The model
incorporates the appropriate actinic solar spectrum, thereby properly
weighting the different rates of photolysis of NO&lt;sub&gt;3&lt;/sub&gt;&lt;sup&gt;&amp;minus;&lt;/sup&gt;
and NO&lt;sub&gt;2&lt;/sub&gt;&lt;sup&gt;&amp;minus;&lt;/sup&gt;. This is important since the immediate precursor
for NO, for example, NO&lt;sub&gt;2&lt;/sub&gt;&lt;sup&gt;&amp;minus;&lt;/sup&gt;, absorbs at wavelengths longer
than nitrate itself. Finally, one-dimensional model simulations indicate
that both gas phase boundary layer NO and NO&lt;sub&gt;2&lt;/sub&gt; exhibit a
negative concentration gradient as a function of height although
[NO]/[NO&lt;sub&gt;2&lt;/sub&gt;] are approximately constant. This gradient is primarily
attributed to gas phase reactions of NO&lt;sub&gt;x&lt;/sub&gt; with halogens oxides (i.e. as BrO
and IO), HO&lt;sub&gt;x&lt;/sub&gt;, and hydrocarbons, such as CH&lt;sub&gt;3&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt;.</abstract>
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</article>

