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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>9</volume_number>
		<issue_number>5</issue_number>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/acpd-9-20371-2009</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/9/20371/2009/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/9/20371/2009/acpd-9-20371-2009.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/9/20371/2009/acpd-9-20371-2009.pdf</fulltext_pdf>
	<start_page>20371</start_page>
	<end_page>20406</end_page>
	<publication_date>2009-09-29</publication_date>
	<article_title content_type="html">Summertime NO&lt;sub&gt;x&lt;/sub&gt; measurements during the CHABLIS campaign: can source and sink estimates unravel observed diurnal cycles?</article_title>
	<authors>
		<author numeration="1" affiliations="1,5">
			<name>S. J.-B. Bauguitte</name>
			<email>s.bauguitte@bas.ac.uk</email>
		</author>
		<author numeration="2" affiliations="2,6">
			<name>W. J. Bloss</name>
		</author>
		<author numeration="3" affiliations="3">
			<name>M. J. Evans</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>R. A. Salmon</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>P. S. Anderson</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>A. E. Jones</name>
		</author>
		<author numeration="7" affiliations="2,7">
			<name>J. D. Lee</name>
		</author>
		<author numeration="8" affiliations="4,8">
			<name>A. Saiz-Lopez</name>
		</author>
		<author numeration="9" affiliations="1">
			<name>H. K. Roscoe</name>
		</author>
		<author numeration="10" affiliations="1">
			<name>E. W. Wolff</name>
		</author>
		<author numeration="11" affiliations="4,9">
			<name>J. M. C. Plane</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">British Antarctic Survey, Natural Environment Research Council, High Cross, Madingley Road, Cambridge, CB3 0ET, UK</affiliation>
		<affiliation numeration="2" content_type="html">School of Chemistry, University of Leeds, Leeds, LS2 9JT, UK</affiliation>
		<affiliation numeration="3" content_type="html">School of Earth and the Environment, University of Leeds, Leeds, LS2 9JT, UK</affiliation>
		<affiliation numeration="4" content_type="html">School of Environmental Sciences, UEA, Norwich, NR4 7TJ, UK</affiliation>
		<affiliation numeration="5" content_type="html">now at: Facility for Airborne Atmospheric Measurements, NERC, Cranfield, Bedfordshire, MK43 0AL, UK</affiliation>
		<affiliation numeration="6" content_type="html">now at: School of Geography, Earth and Environmental Sciences, University of Birmingham, Edgbaston, B15 2TT, UK</affiliation>
		<affiliation numeration="7" content_type="html">now at: Department of Chemistry, University of York, York, YO10 5DD, UK</affiliation>
		<affiliation numeration="8" content_type="html">now at: Atomic and Molecular Physics Division, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA</affiliation>
		<affiliation numeration="9" content_type="html">now at: School of Chemistry, University of Leeds, Leeds, LS2 9JT, UK</affiliation>
	</affiliations>
	<abstract content_type="html">NO&lt;sub&gt;x&lt;/sub&gt; measurements were conducted at the Halley Research Station,
Antarctica, during the austral summer period 1 January–10 February 2005. A clear
NO&lt;sub&gt;x&lt;/sub&gt; diurnal cycle was observed with minimum concentrations close to
instrumental detection limit (5 pptv) measured between 04:00–05:00 GMT.
NO&lt;sub&gt;x&lt;/sub&gt; concentrations peaked (24 pptv) between 19:00–20:00 GMT,
approximately 5 h after local solar noon. An optimised box model of
NO&lt;sub&gt;x&lt;/sub&gt; concentrations based on production from in-snow nitrate photolysis
and chemical loss derives a mean noon emission rate of
3.48&amp;times;10&lt;sup&gt;8&lt;/sup&gt; molecules cm&lt;sup&gt;&amp;minus;2&lt;/sup&gt; s&lt;sup&gt;&amp;minus;1&lt;/sup&gt;, assuming a 100 m boundary layer
mixing height, and a relatively short NO&lt;sub&gt;x&lt;/sub&gt; lifetime of ~6.4 h.
This emission rate compares to directly measured values ranging from 1.7 to
3.4&amp;times;10&lt;sup&gt;8&lt;/sup&gt; molecules cm&lt;sup&gt;&amp;minus;2&lt;/sup&gt; s&lt;sup&gt;&amp;minus;1&lt;/sup&gt; made on 3 days at the
end of the study period. Calculations of the maximum rate of NO&lt;sub&gt;2&lt;/sub&gt; loss
via a variety of conventional HO&lt;sub&gt;x&lt;/sub&gt; and halogen oxidation processes show
that the lifetime of NO&lt;sub&gt;x&lt;/sub&gt; is predominantly controlled by halogen
processing, namely BrNO&lt;sub&gt;3&lt;/sub&gt; and INO&lt;sub&gt;3&lt;/sub&gt; gas-phase formation and their
subsequent heterogeneous uptake, with a potential smaller contribution from
HNO&lt;sub&gt;4&lt;/sub&gt; formation and uptake. Furthermore the presence of halogen oxides
is shown to significantly perturb NO&lt;sub&gt;x&lt;/sub&gt; concentrations by decreasing the
NO/NO&lt;sub&gt;2&lt;/sub&gt; ratio. We conclude that in coastal Antarctica, the potential
ozone production efficiency of NO&lt;sub&gt;x&lt;/sub&gt; emitted from the snowpack is
mitigated by the more rapid NO&lt;sub&gt;x&lt;/sub&gt; loss due to halogen nitrate hydrolysis.
These results suggest that the role of halogen oxides need to be considered
when interpreting the isotopic signature of nitrate impurities held within
snow and ice.</abstract>
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