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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>5</volume_number>
		<issue_number>6</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/acpd-5-12373-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/12373/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/12373/2005/acpd-5-12373-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/12373/2005/acpd-5-12373-2005.pdf</fulltext_pdf>
	<start_page>12373</start_page>
	<end_page>12401</end_page>
	<publication_date>2005-11-28</publication_date>
	<article_title content_type="html">On the ability of chemical transport models to simulate the vertical structure of the N&lt;sub&gt;2&lt;/sub&gt;O, NO&lt;sub&gt;2&lt;/sub&gt; and HNO&lt;sub&gt;3&lt;/sub&gt; species in the mid-latitude stratosphere</article_title>
	<authors>
		<author numeration="1" affiliations="1,2">
			<name>G. Berthet</name>
			<email>g.berthet@damtp.cam.ac.uk</email>
		</author>
		<author numeration="2" affiliations="2">
			<name>N. Huret</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>F. Lefèvre</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>G. Moreau</name>
		</author>
		<author numeration="5" affiliations="2">
			<name>C. Robert</name>
		</author>
		<author numeration="6" affiliations="2">
			<name>M. Chartier</name>
		</author>
		<author numeration="7" affiliations="2">
			<name>L. Pomathiod</name>
		</author>
		<author numeration="8" affiliations="2">
			<name>M. Pirre</name>
		</author>
		<author numeration="9" affiliations="2">
			<name>V. Catoire</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Service d’Aéronomie, Institut Pierre-Simon Laplace, F-75252 Paris, France</affiliation>
		<affiliation numeration="2" content_type="html">Laboratoire de Physique et Chimie de l’Environnement, F-45071 Orléans, France</affiliation>
	</affiliations>
	<abstract content_type="html">In this paper we study the impact of the modelling of N&lt;sub&gt;2&lt;/sub&gt;O on the
simulation of NO&lt;sub&gt;2&lt;/sub&gt; and HNO&lt;sub&gt;3&lt;/sub&gt; by comparing in situ vertical profiles
measured at mid-latitudes with the results of the Reprobus 3-D CTM
(Three-dimensional Chemical Transport Model) computed with the kinetic
parameters from the JPL recommendation in 2002. The analysis of the measured
in situ profile of N&lt;sub&gt;2&lt;/sub&gt;O shows particular features indicating different air mass
origins. The measured N&lt;sub&gt;2&lt;/sub&gt;O, NO&lt;sub&gt;2&lt;/sub&gt; and HNO&lt;sub&gt;3&lt;/sub&gt; profiles are not
satisfyingly reproduced by the CTM when computed using the current 6-hourly
ECMWF operational analysis. Improving the simulation of N&lt;sub&gt;2&lt;/sub&gt;O transport
allows us to calculate quantities of NO&lt;sub&gt;2&lt;/sub&gt; and HNO&lt;sub&gt;3&lt;/sub&gt; in reasonable
agreement with observations. This is achieved using 3-hourly winds obtained
from ECMWF forecasts. The best agreement is obtained by constraining a
one-dimensional version of the model with the observed N&lt;sub&gt;2&lt;/sub&gt;O. This study
shows that modelling the NO&lt;sub&gt;y&lt;/sub&gt; partitioning with better accuracy relies
at least on a correct simulation of N&lt;sub&gt;2&lt;/sub&gt;O and thus of total NO&lt;sub&gt;y&lt;/sub&gt;.</abstract>
	<references>
	</references>
</article>

