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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>4</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/acpd-5-7457-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/7457/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/7457/2005/acpd-5-7457-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/7457/2005/acpd-5-7457-2005.pdf</fulltext_pdf>
	<start_page>7457</start_page>
	<end_page>7496</end_page>
	<publication_date>2005-08-26</publication_date>
	<article_title content_type="html">On the observation of mesospheric air inside the arctic stratospheric polar vortex in early 2003</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>A. Engel</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>T. Möbius</name>
		</author>
		<author numeration="3" affiliations="1,6">
			<name>H.-P. Haase</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>H. Bönisch</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>T. Wetter</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>U. Schmidt</name>
		</author>
		<author numeration="7" affiliations="2">
			<name>I. Levin</name>
		</author>
		<author numeration="8" affiliations="3">
			<name>T. Reddmann</name>
		</author>
		<author numeration="9" affiliations="3">
			<name>H. Oelhaf</name>
		</author>
		<author numeration="10" affiliations="3">
			<name>G. Wetzel</name>
		</author>
		<author numeration="11" affiliations="4">
			<name>K. Grunow</name>
		</author>
		<author numeration="12" affiliations="5">
			<name>N. Huret</name>
		</author>
		<author numeration="13" affiliations="5">
			<name>M. Pirre</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institut für Atmosphäre und Umwelt, J. W. Goethe Universität Frankfurt, Frankfurt, Germany</affiliation>
		<affiliation numeration="2" content_type="html">Institut für Umweltphysik, Ruprecht – Karls Universität Heidelberg, Heidelberg, Germany</affiliation>
		<affiliation numeration="3" content_type="html">Institut für Meteorologie und Klimaforschung, Forschungszentrum Karlsruhe, Karlsruhe, Germany</affiliation>
		<affiliation numeration="4" content_type="html">Institut für Meteorologie, Freie Universität Berlin, Berlin, Germany</affiliation>
		<affiliation numeration="5" content_type="html">Laboratoire de Physique et Chimie de l’Environnement, CNRS and Université d’Orléans, Orléans, France</affiliation>
		<affiliation numeration="6" content_type="html">now at: DEKA Bank, Frankfurt, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">During several balloon flights inside the Arctic polar vortex in early 2003,
unusual trace gas distributions were observed, which indicate a strong
influence of mesospheric air in the stratosphere. The tuneable diode laser
(TDL) instrument SPIRALE (Spectroscopie InFrarouge par Absorption de Lasers
Embarqu&amp;#233;s) measured unusually high CO values (up to 600 ppb) on 27&amp;nbsp;January
at about 30 km altitude. The cryosampler BONBON sampled air masses with
very high molecular Hydrogen, extremely low SF&lt;sub&gt;6&lt;/sub&gt; and enhanced CO values
on 6&amp;nbsp;March at about 25 km altitude. Finally, the MIPAS (Michelson
Interferometer for Passive Atmospheric Sounding) Fourier Transform Infra-Red
(FTIR) spectrometer showed NO&lt;sub&gt;y&lt;/sub&gt; values which are significantly higher
than NO&lt;sub&gt;y&lt;/sub&gt;* (the NO&lt;sub&gt;y&lt;/sub&gt; derived from a 
correlation between N&lt;sub&gt;2&lt;/sub&gt;O and
NO&lt;sub&gt;y&lt;/sub&gt; under undisturbed conditions), on 21 and 22&amp;nbsp;March in a layer
centred at 22 km altitude. Thus, the mesospheric air seems to have been
present in a layer descending from about 30 km in late January to 25 km
altitude in early March and about 22 km altitude on 20&amp;nbsp;March. We present
corroborating evidence from a model study using the KASIMA (KArlsruhe
Simulation model of the Middle Atmosphere) model that also shows a layer of
mesospheric air, which descended into the stratosphere in November and early
December 2002, before the minor warming which occurred in late December 2002
lead to a descent of upper stratospheric air, cutting of a layer in which
mesospheric air is present. This layer then descended inside the vortex over
the course of the winter. The same feature is found in trajectory
calculations, based on a large number of trajectories started in the
vicinity of the observations on 6&amp;nbsp;March. Based on the difference between the
mean age derived from SF&lt;sub&gt;6&lt;/sub&gt; (which has an irreversible mesospheric loss)
and from CO&lt;sub&gt;2&lt;/sub&gt; (whose mesospheric loss is much smaller and reversible) we
estimate that the fraction of mesospheric air in the layer observed on 6&amp;nbsp;March,
must have been somewhere between 35% and 100%.</abstract>
	<references>
	</references>
</article>

