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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ACPD</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics Discussions</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACPD</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7375</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/acpd-8-18727-2008</article-id>
<title-group>
<article-title>Implications of Lagrangian transport for coupled chemistry-climate simulations</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Stenke</surname>
<given-names>A.</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>Dameris</surname>
<given-names>M.</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>Grewe</surname>
<given-names>V.</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>Garny</surname>
<given-names>H.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Deutsches Zentrum für Luft- und Raumfahrt (DLR), Institut für Physik der Atmosphäre, Oberpfaffenhofen, Germany</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Meteorological Institute, University of Munich, Munich, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>31</day>
<month>10</month>
<year>2008</year>
</pub-date>
<volume>8</volume>
<issue>5</issue>
<fpage>18727</fpage>
<lpage>18764</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>
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<self-uri xlink:href="http://www.atmos-chem-phys-discuss.net/8/18727/2008/acpd-8-18727-2008.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys-discuss.net/8/18727/2008/acpd-8-18727-2008.pdf</self-uri>
<abstract>
<p>For the first time a purely Lagrangian transport algorithm is
  applied in a fully coupled chemistry-climate model (CCM). We use the
  Lagrangian scheme ATTILA for the transport of water vapour, cloud
  water and chemical trace species in the ECHAM4.L39(DLR)/CHEM
  (E39C) CCM. The advantage of the Lagrangian approach is that it is
  numerically non-diffusive and therefore maintains steeper and more
  realistic gradients than the operational semi-Lagrangian transport
  scheme. In case of radiatively active species changes in the
  simulated distributions feed back to model dynamics which in turn
  affect the modelled transport. The implications of the Lagrangian
  transport scheme for stratospheric model dynamics and tracer
  distributions in the upgraded model version E39C-ATTILA (E39C-A) are
  evaluated by comparison with observations and results of the E39C
  model with the operational semi-Lagrangian advection scheme. We find
  that several deficiencies in stratospheric dynamics in E39C seem to
  originate from a pronounced modelled wet bias and an associated cold
  bias in the extra-tropical lowermost stratosphere. The reduction of
  the simulated moisture and temperature bias in E39C-A leads to a
  significant advancement of stratospheric dynamics in terms of the
  mean state as well as annual and interannual variability. As a
  consequence of the favourable numerical characteristics of the
  Lagrangian transport scheme and the improved model dynamics, E39C-A
  generally shows more realistic stratospheric tracer distributions:
  Compared to E39C high stratospheric chlorine (Cl&lt;sub&gt;y&lt;/sub&gt;)
  concentrations extend further downward and agree now well with
  analyses derived from observations. Therefore E39C-A realistically
  covers the altitude of maximum ozone depletion in the stratosphere.
  The location of the ozonopause, i.e. the transition from low
  tropospheric to high stratospheric ozone values, is also clearly
  improved in E39C-A.  Furthermore, the simulated temporal evolution
  of stratospheric Cl&lt;sub&gt;y&lt;/sub&gt; in the past is realistically reproduced
  which is an important step towards a more reliable projection of
  future changes, especially of stratospheric ozone.</p>
</abstract>
<counts><page-count count="38"/></counts>
</article-meta>
</front>
<body/>
<back>
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