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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>7</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2007</publication_year>
	</journal>
	<doi>10.5194/acpd-7-9385-2007</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/7/9385/2007/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/7/9385/2007/acpd-7-9385-2007.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/7/9385/2007/acpd-7-9385-2007.pdf</fulltext_pdf>
	<start_page>9385</start_page>
	<end_page>9417</end_page>
	<publication_date>2007-07-02</publication_date>
	<article_title content_type="html">On the vertical distribution of boundary layer halogens over coastal Antarctica: implications for O&lt;sub&gt;3&lt;/sub&gt;, HO&lt;sub&gt;x&lt;/sub&gt;, NO&lt;sub&gt;x&lt;/sub&gt; and the Hg lifetime</article_title>
	<authors>
		<author numeration="1" affiliations="1,2">
			<name>A. Saiz-Lopez</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>J. M. C. Plane</name>
			<email>j.m.c.plane@leeds.ac.uk</email>
		</author>
		<author numeration="3" affiliations="1">
			<name>A. S. Mahajan</name>
		</author>
		<author numeration="4" affiliations="3">
			<name>P. S. Anderson</name>
		</author>
		<author numeration="5" affiliations="3">
			<name>S. J.-B. Bauguitte</name>
		</author>
		<author numeration="6" affiliations="3">
			<name>A. E. Jones</name>
		</author>
		<author numeration="7" affiliations="3">
			<name>H. K. Roscoe</name>
		</author>
		<author numeration="8" affiliations="3">
			<name>R. A. Salmon</name>
		</author>
		<author numeration="9" affiliations="1,4">
			<name>W. J. Bloss</name>
		</author>
		<author numeration="10" affiliations="1,5">
			<name>J. D. Lee</name>
		</author>
		<author numeration="11" affiliations="1">
			<name>D. E. Heard</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">NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA</affiliation>
		<affiliation numeration="3" content_type="html">British Antarctic Survey, National Environment Research Council, Cambridge, UK</affiliation>
		<affiliation numeration="4" content_type="html">now at: School of Geography, Earth &amp; Environmental Sciences, University of Birmingham, Edgbaston, Birmingham, UK</affiliation>
		<affiliation numeration="5" content_type="html">now at: Department of Chemistry, University of York, Heslington, York, UK</affiliation>
	</affiliations>
	<abstract content_type="html">A one-dimensional chemical transport model has been developed to investigate
the vertical gradients of bromine and iodine compounds in the Antarctic
coastal boundary layer. The model has been applied to interpret recent
year-round observations of iodine and bromine monoxides (IO and BrO) at
Halley Station, Antarctica. The model requires an equivalent I atom flux of
~10&lt;sup&gt;9&lt;/sup&gt; molecule cm&lt;sup&gt;&amp;minus;2&lt;/sup&gt; s&lt;sup&gt;&amp;minus;1&lt;/sup&gt; from the snowpack in order to
account for the measured IO levels, which are up to 20 ppt during spring.
Using the current knowledge of gas-phase iodine chemistry, the model
predicts significant gradients in the vertical distribution of iodine
species. However, recent ground-based and satellite observations of IO imply
that the radical is well-mixed in the boundary layer, indicating a longer
than expected atmospheric lifetime for the radical. This can be modelled by
including photolysis of the higher iodine oxides (I&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt;,
I&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;3&lt;/sub&gt;, I&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;4&lt;/sub&gt; and I&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt;), and rapid recycling of
HOI and INO&lt;sub&gt;3&lt;/sub&gt; through sea-salt aerosol. The model also predicts
significant concentrations (up to 25 ppt) of I&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; in the
lowest 10 m of the boundary layer, which could lead to the formation of
ultrafine iodine oxide aerosols. Heterogeneous chemistry involving sea-salt
aerosol is also necessary to account for the vertical profile of BrO. Iodine
chemistry causes a large increase (typically more than 3-fold) in the rate
of O&lt;sub&gt;3&lt;/sub&gt; depletion in the BL, compared with bromine chemistry alone. Rapid
entrainment of O&lt;sub&gt;3&lt;/sub&gt; from the free troposphere is required to account for
the observation that on occasion there is little O&lt;sub&gt;3&lt;/sub&gt; depletion at the
surface in the presence of high concentrations of IO and BrO. The halogens
also cause significant changes to the vertical profiles of HO and HO&lt;sub&gt;2&lt;/sub&gt;
and the NO&lt;sub&gt;2&lt;/sub&gt;/NO ratio. The average Hg&lt;sup&gt;0&lt;/sup&gt; lifetime against oxidation
is also predicted to be about 10 h during springtime. Overall, our
results show that halogens profoundly influence the oxidizing capacity of
the Antarctic troposphere.</abstract>
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</article>

