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<!DOCTYPE article SYSTEM "http://www.atmos-chem-phys-discuss.net/inc/acpd/copernicus.dtd">
<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>5</volume_number>
		<issue_number>1</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/acpd-5-937-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/937/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/937/2005/acpd-5-937-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/937/2005/acpd-5-937-2005.pdf</fulltext_pdf>
	<start_page>937</start_page>
	<end_page>960</end_page>
	<publication_date>2005-02-18</publication_date>
	<article_title content_type="html">Atmospheric trends of the halon gases from polar firn air</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>C. E. Reeves</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>W. T. Sturges</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>G. A. Sturrock</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>K. Preston</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>D. E. Oram</name>
		</author>
		<author numeration="6" affiliations="2">
			<name>J. Schwander</name>
		</author>
		<author numeration="7" affiliations="3">
			<name>R. Mulvaney</name>
		</author>
		<author numeration="8" affiliations="4">
			<name>J.-M. Barnola</name>
		</author>
		<author numeration="9" affiliations="4">
			<name>J. Chappellez</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">School of Environmental Sciences, University of East Anglia, Norwich, NR4 7TJ, UK</affiliation>
		<affiliation numeration="2" content_type="html">Physics Institute, University of Berne, Berne, Switzerland</affiliation>
		<affiliation numeration="3" content_type="html">British Antarctic Survey, Natural Environment Research Council, Cambridge, UK</affiliation>
		<affiliation numeration="4" content_type="html">CNRS Laboratoire de Glaciologie et Geophysique de l’Environnement, Saint Martin d’Heres, France</affiliation>
	</affiliations>
	<abstract content_type="html">Four halons (H-1301, H-1211, H-2402 and H-1202) have been measured in air
samples collected from polar firn from Dome Concordia (Dome C), Antarctica,
from Devon Island, Canada and the North Greenland Ice Core Project (NGRIP)
site, Greenland. H-2402 and H-1202 are reported for the first time in firn
air. The depth profiles show the concentrations of all four halons to be
zero at the base of the firn thus demonstrating their entirely anthropogenic
origin. This is the first evidence of this for H-2402 and H-1202. A 2-D
atmospheric model was run to produce historical trends in the atmospheric
concentrations at the firn sites, which were then input into a firn
diffusion model to produce concentration depth profiles for comparison with
the measurements. The firn measurements provide constraints on the
atmospheric concentrations in both hemispheres which allow the global
emission rates and their latitudinal distribution in the atmospheric model
to be evaluated. Global emission trends previously determined from
measurements at Cape Grim are found to be consistent with the firn data.
Further emissions of H-1202 in recent years (late 1980s onwards) are likely
to have come from latitudes mostly south of 40&amp;deg; N, but emissions prior to
that may have come from further north. Emissions of H-1211 may also have
shifted to latitudes south of 40&amp;deg; N during the late 1980s. The firn data
is used to derive atmospheric trends in total organic bromine in the form of
halons for both polar regions.</abstract>
	<references>
	</references>
</article>

