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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>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7324</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-4-1085-2004</article-id>
<title-group>
<article-title>Secondary maxima in ozone profiles</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Lemoine</surname>
<given-names>R.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Royal Meteorological Institute of Belgium, 3, Avenue Circulaire, 1180 Brussels, Belgium</addr-line>
</aff>
<pub-date pub-type="epub">
<day>08</day>
<month>07</month>
<year>2004</year>
</pub-date>
<volume>4</volume>
<issue>4</issue>
<fpage>1085</fpage>
<lpage>1096</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2004 R. Lemoine</copyright-statement>
<copyright-year>2004</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Generic License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by-nc-sa/2.5/">https://creativecommons.org/licenses/by-nc-sa/2.5/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://acp.copernicus.org/articles/4/1085/2004/acp-4-1085-2004.html">This article is available from https://acp.copernicus.org/articles/4/1085/2004/acp-4-1085-2004.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/articles/4/1085/2004/acp-4-1085-2004.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/4/1085/2004/acp-4-1085-2004.pdf</self-uri>
<abstract>
<p>Ozone profiles from balloon soundings as well as SAGEII ozone
  profiles were used to detect anomalous large ozone concentrations of
  ozone in the lower stratosphere. These secondary ozone maxima are
  found to be the result of differential advection of ozone-poor and
  ozone-rich air associated with Rossby wave breaking events. The
  frequency and intensity of secondary ozone maxima and their
  geographical distribution is presented. The occurrence and amplitude
  of ozone secondary maxima is connected to ozone variability and trend
  at Uccle and account for a large part of the total ozone and lower
  stratospheric ozone variability.</p>
</abstract>
<counts><page-count count="12"/></counts>
</article-meta>
</front>
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<back>
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</article>