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<article language="en">
	<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>6</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acp-6-1135-2006</doi>
	<article_url>http://www.atmos-chem-phys.net/6/1135/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys.net/6/1135/2006/acp-6-1135-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys.net/6/1135/2006/acp-6-1135-2006.pdf</fulltext_pdf>
	<start_page>1135</start_page>
	<end_page>1153</end_page>
	<publication_date>2006-04-05</publication_date>
	<article_title content_type="html">OH and HO&lt;sub&gt;2&lt;/sub&gt; chemistry during NAMBLEX: roles of oxygenates, halogen oxides and heterogeneous uptake</article_title>
	<authors>
		<author numeration="1" affiliations="1,7">
			<name>R. Sommariva</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>W. J. Bloss</name>
		</author>
		<author numeration="3" affiliations="3">
			<name>N. Brough</name>
		</author>
		<author numeration="4" affiliations="4">
			<name>N. Carslaw</name>
		</author>
		<author numeration="5" affiliations="6">
			<name>M. Flynn</name>
		</author>
		<author numeration="6" affiliations="2">
			<name>A.-L. Haggerstone</name>
		</author>
		<author numeration="7" affiliations="1">
			<name>D. E. Heard</name>
		</author>
		<author numeration="8" affiliations="2">
			<name>J. R. Hopkins</name>
		</author>
		<author numeration="9" affiliations="1,8">
			<name>J. D. Lee</name>
		</author>
		<author numeration="10" affiliations="2">
			<name>A. C. Lewis</name>
		</author>
		<author numeration="11" affiliations="6">
			<name>G. McFiggans</name>
		</author>
		<author numeration="12" affiliations="5">
			<name>P. S. Monks</name>
		</author>
		<author numeration="13" affiliations="3">
			<name>S. A. Penkett</name>
		</author>
		<author numeration="14" affiliations="1">
			<name>M. J. Pilling</name>
		</author>
		<author numeration="15" affiliations="3">
			<name>J. M. C. Plane</name>
		</author>
		<author numeration="16" affiliations="1">
			<name>K. A. Read</name>
		</author>
		<author numeration="17" affiliations="3">
			<name>A. Saiz-Lopez</name>
		</author>
		<author numeration="18" affiliations="5,9">
			<name>A. R. Rickard</name>
		</author>
		<author numeration="19" affiliations="6">
			<name>P. I. Williams</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">School of Chemistry, University of Leeds, Leeds, UK</affiliation>
		<affiliation numeration="2" content_type="html">Department of Chemistry, University of York, York, UK</affiliation>
		<affiliation numeration="3" content_type="html">School of Environmental Sciences, University of East Anglia, Norwich, UK</affiliation>
		<affiliation numeration="4" content_type="html">Environment Department, University of York, York, UK</affiliation>
		<affiliation numeration="5" content_type="html">Department of Chemistry, University of Leicester, Leicester, UK</affiliation>
		<affiliation numeration="6" content_type="html">School of Earth, Atmospheric &amp; Environmental Sciences, University of Manchester, Manchester, UK</affiliation>
		<affiliation numeration="7" content_type="html">now at: Earth System Research Laboratory, National Oceanic and Atmospheric Administration, Boulder, CO, USA</affiliation>
		<affiliation numeration="8" content_type="html">now at: Department of Chemistry, University of York, York, UK</affiliation>
		<affiliation numeration="9" content_type="html">now at: School of Chemistry, University of Leeds, Leeds, UK</affiliation>
	</affiliations>
	<abstract content_type="html">Several zero-dimensional box-models with different levels of
chemical complexity, based on the Master Chemical Mechanism (MCM),
have been used to study the chemistry of OH and HO&lt;sub&gt;2&lt;/sub&gt;
in a coastal environment in the Northern Hemisphere. The models
were constrained to and compared with measurements made during the
NAMBLEX campaign (Mace Head, Ireland) in summer 2002.

&lt;P  style=&quot;line-height: 20px;&quot;&gt;
The base models, which were constrained to measured CO,
CH&lt;sub&gt;4&lt;/sub&gt; and NMHCs, were able to reproduce [OH] within
25%, but overestimated [HO&lt;sub&gt;2&lt;/sub&gt;] by about a factor of 2.
Agreement was improved when the models were constrained to
oxygenated compounds (acetaldehyde, methanol and acetone),
highlighting their importance for the radical budget. When the
models were constrained to measured halogen monoxides (IO,
BrO) and used a more detailed, measurements-based,
treatment to describe the heterogeneous uptake, modelled
[OH] increased by up to 15% and [HO&lt;sub&gt;2&lt;/sub&gt;] decreased by
up to 30%. The actual impact of halogen monoxides on the modelled
concentrations of HO&lt;sub&gt;x&lt;/sub&gt; was dependant on the uptake
coefficients used for HOI, HOBr and HO&lt;sub&gt;2&lt;/sub&gt;.
Better agreement, within the combined uncertainties of the
measurements and of the model, was achieved when using high uptake
coefficients for HO&lt;sub&gt;2&lt;/sub&gt; and HOI
(&amp;gamma;&lt;sub&gt;HO&lt;sub&gt;2&lt;/sub&gt;&lt;/sub&gt;=1, &amp;gamma;&lt;sub&gt;HOI&lt;/sub&gt;=0.6).

&lt;P  style=&quot;line-height: 20px;&quot;&gt;
A rate of production and destruction analysis of the models
allowed a detailed study of OH and HO&lt;sub&gt;2&lt;/sub&gt; chemistry
under the conditions encountered during NAMBLEX, showing the
importance of oxygenates and of XO (where X=I, Br) as co-reactants for OH and
HO&lt;sub&gt;2&lt;/sub&gt;
and of HOX photolysis as a source for OH.</abstract>
	<references>
	</references>
</article>

