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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ACP</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7324</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-10-3155-2010</article-id>
<title-group>
<article-title>Sensitivity of ensemble Lagrangian reconstructions to assimilated wind time step resolution</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Pisso</surname>
<given-names>I.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Marécal</surname>
<given-names>V.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Legras</surname>
<given-names>B.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Berthet</surname>
<given-names>G.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Laboratoire de Météorologie Dynamique (UMR 8539), ENS – CNRS, Paris, France</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Laboratoire de Physique et Chimie de l&apos;Environnement et de l&apos;Espace (UMR 6115), Université d&apos;Orléans &amp;ndash; CNRS, Orléans, France</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>now at: Research Institute for Global Change, JAMSTEC, Yokohama, Japan</addr-line>
</aff>
<pub-date pub-type="epub">
<day>01</day>
<month>04</month>
<year>2010</year>
</pub-date>
<volume>10</volume>
<issue>7</issue>
<fpage>3155</fpage>
<lpage>3162</lpage>
<permissions>
<license xlink:type="simple">
<license-p>This is an open-access article ditributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.</license-p>
</license>
</permissions>
<self-uri xlink:href="http://www.atmos-chem-phys.net/10/3155/2010/acp-10-3155-2010.html">This article is available from http://www.atmos-chem-phys.net/10/3155/2010/acp-10-3155-2010.html</self-uri>
<self-uri xlink:href="http://www.atmos-chem-phys.net/10/3155/2010/acp-10-3155-2010.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/10/3155/2010/acp-10-3155-2010.pdf</self-uri>
<abstract>
<p>We study the impact of temporal and spatial resolution and changes in modelled
meteorological winds in the context of diffusive ensemble Lagrangian
reconstructions. In situ tracer measurements are modelled based on coarse
resolution global 3-D tracer distributions from a chemistry-transport model
and on different time series of meteorological wind fields including a
special set of 1-hourly analysed winds which is compared with 3 and 6-hourly
operational analysed winds and with 3-hourly ERA-interim reanalysis.
Increasing the time resolution of the advecting winds from three to one hour
using the operational winds provides an improvement on diffusive
reconstructions in the period studied but smaller than that obtained from six
to three hours. The positive impact of using 1-hourly winds is similar to
that obtained using ERA-Interim 3-hourly winds instead of the 3-hourly ECMWF
operational analysis for the same period. This study sets out a technique to
quantify differences in time series of meteorological wind fields here
applied to assess the optimal space and time resolutions for ensemble
Lagrangian reconstructions in the lower stratosphere.</p>
</abstract>
<counts><page-count count="8"/></counts>
</article-meta>
</front>
<body/>
<back>
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</back>
</article>