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<!DOCTYPE article SYSTEM "http://www.atmos-chem-phys.net/inc/acp/copernicus.dtd">
<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>6</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acp-6-1513-2006</doi>
	<article_url>http://www.atmos-chem-phys.net/6/1513/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys.net/6/1513/2006/acp-6-1513-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys.net/6/1513/2006/acp-6-1513-2006.pdf</fulltext_pdf>
	<start_page>1513</start_page>
	<end_page>1528</end_page>
	<publication_date>2006-05-11</publication_date>
	<article_title content_type="html">Measurements and modelling of I&lt;sub&gt;2&lt;/sub&gt;, IO, OIO, BrO and NO&lt;sub&gt;3&lt;/sub&gt; in the mid-latitude marine boundary layer</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>A. Saiz-Lopez</name>
		</author>
		<author numeration="2" affiliations="2">
			<name>J. A. Shillito</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>H. Coe</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>J. M. C. Plane</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">School of Environmental Sciences, University of East Anglia, Norwich, UK</affiliation>
		<affiliation numeration="2" content_type="html">School of Earth, Atmospheric &amp; Environmental Sciences, University of Manchester, Manchester, UK</affiliation>
	</affiliations>
	<abstract content_type="html">Time series observations of molecular iodine (I&lt;sub&gt;2&lt;/sub&gt;), iodine
oxides (IO, OIO), bromine oxide (BrO), and the nitrate radical
(NO&lt;sub&gt;3&lt;/sub&gt;) in the mid-latitude coastal marine boundary layer
(MBL) are reported. Measurements were made using a new long-path
DOAS instrument during a summertime campaign at Mace Head on the
&lt;i&gt;B&lt;/i&gt;&lt;sup&gt;3&lt;/sup&gt;&amp;Pi;(0&lt;sup&gt;+&lt;/sup&gt;&lt;sub&gt;u&lt;/sub&gt;)-&lt;i&gt;X&lt;/i&gt;&lt;sup&gt;1&lt;/sup&gt;&amp;Sigma;&lt;sup&gt;+&lt;/sup&gt;&lt;sub&gt;g&lt;/sub&gt; electronic transition
between 535 and 575 nm.  The I&lt;sub&gt;2&lt;/sub&gt; mixing ratio was found to
vary from below the detection limit (~5 ppt) up to a nighttime
maximum of 93 ppt. Along with I&lt;sub&gt;2&lt;/sub&gt;, observations of IO, OIO
and NO&lt;sub&gt;3&lt;/sub&gt; were also made during the night.  Surprisingly, IO
and OIO were detected at mixing ratios up to 2.5 and 10.8 ppt,
respectively.  A model is employed to show that the reaction
between I&lt;sub&gt;2&lt;/sub&gt; and NO&lt;sub&gt;3&lt;/sub&gt; is the likely nighttime source of
these radicals.  The BrO mixing ratio varied from below the
detection limit at night (~1 ppt) to a maximum of 6 ppt in the
first hours after sunrise.  A bromine chemistry model is used to
simulate the diurnal behaviour of the BrO radical, demonstrating the
importance of halogen recycling through sea-salt aerosol. In the
same campaign a zenith sky DOAS was employed to determine the column
density variation of NO&lt;sub&gt;3&lt;/sub&gt; as a function of solar zenith angle
(SZA) during sunrise, from which vertical profiles of NO&lt;sub&gt;3&lt;/sub&gt;
through the troposphere were obtained.  On several occasions a
positive gradient of NO&lt;sub&gt;3&lt;/sub&gt; was observed over the first 2 km,
possibly due to dimethyl sulphide (DMS) removing NO&lt;sub&gt;3&lt;/sub&gt; at the
ocean surface.</abstract>
	<references>
	</references>
</article>

