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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>6</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acpd-6-6695-2006</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/6/6695/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/6/6695/2006/acpd-6-6695-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/6/6695/2006/acpd-6-6695-2006.pdf</fulltext_pdf>
	<start_page>6695</start_page>
	<end_page>6722</end_page>
	<publication_date>2006-07-17</publication_date>
	<article_title content_type="html">Mid-latitude ozone changes: studies with a 3-D CTM forced by ERA-40 analyses</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>W. Feng</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>M. P. Chipperfield</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>M. Dorf</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>K. Pfeilsticker</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institute for Atmospheric Science, School of Earth and Environment, University of Leeds, Leeds, UK</affiliation>
		<affiliation numeration="2" content_type="html">Institute für Umweltphysik, University of Heidelberg, Heidelberg, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">We have used an off-line three-dimensional (3-D) chemical
transport model (CTM) to study long-term changes in stratospheric
O&lt;sub&gt;3&lt;/sub&gt;. The model was run from 1977&amp;ndash;2004 and forced by ECMWF ERA-40
and operational analyses. Model runs were performed to
examine the impact of increasing halogens and additional
stratospheric bromine from short-lived source gases.
The analyses capture much of the observed interannual variability
in column ozone, but there are also unrealistic features. In
particular the ERA-40 analyses cause a large positive anomaly
in northern hemisphere (NH) column O&lt;sub&gt;3&lt;/sub&gt; in the late 1980s. Also, the
change from ERA-40 to operational winds at the start of 2002
introduces abrupt changes in some model fields which affect
analysis of trends.
The model reproduces the observed column increase in NH mid-latitudes
from the mid 1990s. Analysis of a run with fixed halogens
shows that this increase is not due to
a significant decrease in halogen-induced
loss, i.e.&amp;nbsp;is not an indication of recovery. The model predicts
only a small decrease in halogen-induced loss after 1999.
In the upper stratosphere, despite the modelled turnover of chlorine
around 1999, O&lt;sub&gt;3&lt;/sub&gt; does not increase to the effects of increasing
ECMWF temperatures, decreasing modelled CH&lt;sub&gt;4&lt;/sub&gt; at this
altitude, and abrupt
changes to the SH temperatures at the end of the ERA-40 period.
The impact of an additional 5 pptv stratospheric bromine from short-lived
species decreases mid-latitude column O&lt;sub&gt;3&lt;/sub&gt; by about 10 DU. However,
the impact on the modelled relative O&lt;sub&gt;3&lt;/sub&gt; anomaly is generally
small except during periods of large volcanic loading.</abstract>
	<references>
	</references>
</article>

