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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>6</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acpd-6-12217-2006</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/6/12217/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/6/12217/2006/acpd-6-12217-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/6/12217/2006/acpd-6-12217-2006.pdf</fulltext_pdf>
	<start_page>12217</start_page>
	<end_page>12266</end_page>
	<publication_date>2006-11-28</publication_date>
	<article_title content_type="html">Contribution of mixing to the upward transport across the TTL</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>P. Konopka</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>G. Günther</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>R. Müller</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>F. H. S. dos Santos</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>C. Schiller</name>
		</author>
		<author numeration="6" affiliations="2">
			<name>F. Ravegnani</name>
		</author>
		<author numeration="7" affiliations="3">
			<name>A. Ulanovsky</name>
		</author>
		<author numeration="8" affiliations="4">
			<name>H. Schlager</name>
		</author>
		<author numeration="9" affiliations="5">
			<name>C. M. Volk</name>
		</author>
		<author numeration="10" affiliations="6">
			<name>S. Viciani</name>
		</author>
		<author numeration="11" affiliations="7">
			<name>L. Pan</name>
		</author>
		<author numeration="12" affiliations="7">
			<name>D.-S. McKenna</name>
		</author>
		<author numeration="13" affiliations="1">
			<name>M. Riese</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Forschungszentrum Jülich (ICG-I: Stratosphere), Germany</affiliation>
		<affiliation numeration="2" content_type="html">CNR-ISAC, Bologna, Italy</affiliation>
		<affiliation numeration="3" content_type="html">CAO, Dolgoprudny, Russia</affiliation>
		<affiliation numeration="4" content_type="html">Institut für Physik der Atmosphäre, DLR Oberpfaffenhofen, Germany</affiliation>
		<affiliation numeration="5" content_type="html">Institut für Meteorologie und Geophysik, Universität Frankfurt, Germany</affiliation>
		<affiliation numeration="6" content_type="html">INOA, Firenze, Italy</affiliation>
		<affiliation numeration="7" content_type="html">National Center for Atmospheric Research, Boulder, CO, USA</affiliation>
	</affiliations>
	<abstract content_type="html">During the second part of the
TROCCINOX campaign that took place in Brazil in early 2005,
chemical species were measured on-board of the high altitude research aircraft
Geophysica (ozone, water vapor, NO, NO&lt;sub&gt;y&lt;/sub&gt;, CH&lt;sub&gt;4&lt;/sub&gt; and CO)
in the altitude range up to 20 km (or up to 450 K potential temperature),
i.e.&amp;nbsp;spanning the TTL region roughly extending between 350 and 420 K.

&lt;br&gt;&lt;br&gt;
Analysis of transport across TTL is performed using a new version of the
Chemical Lagrangian Model of the Stratosphere (CLaMS). In this new
version, the stratospheric model has been extended to the earth surface.
Above the tropopause, the isentropic and cross-isentropic advection in CLaMS
is driven by ECMWF winds and heating/cooling rates derived from a radiation
calculation.
Below the tropopause the model smoothly transforms from the isentropic to
hybrid-pressure coordinate and, in this way, takes into account the
effect of large-scale convective transport
as implemented in the ECMWF vertical wind.
As with other CLaMS simulations, the irreversible transport, i.e.&amp;nbsp;mixing,
is controlled by the local horizontal strain and vertical shear rates.

&lt;br&gt;&lt;br&gt;
Stratospheric and tropospheric signatures in the TTL can
be seen both in the observation and in the model.
The composition of air above &amp;asymp;350 K is mainly controlled
by mixing on a time scale of weeks or even months. Based on
CLaMS transport studies where mixing can be completely switched
off, we deduce that vertical mixing, mainly driven by the vertical shear in
the outflow regions of the large-scale convection and in the vicinity
of the subtropical jets, is necessary to understand the upward transport
of the tropospheric air from the main convective outflow around 350 K up
to the tropical tropopause around 380 K. This mechanism is
most effective if the outflow of the mesoscale convective systems
interacts with the subtropical jets.</abstract>
	<references>
	</references>
</article>

