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<!DOCTYPE article SYSTEM "http://www.atmos-chem-phys.net/inc/acp/copernicus.dtd">
<article language="en">
	<journal>
		<journal_title>Atmospheric Chemistry and Physics</journal_title>
		<journal_url>www.atmos-chem-phys.net</journal_url>
		<issn>1680-7316</issn>
		<eissn>1680-7324</eissn>
		<volume_number>4</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2004</publication_year>
	</journal>
	<doi>10.5194/acp-4-1085-2004</doi>
	<article_url>http://www.atmos-chem-phys.net/4/1085/2004/</article_url>
	<abstract_html>http://www.atmos-chem-phys.net/4/1085/2004/acp-4-1085-2004.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys.net/4/1085/2004/acp-4-1085-2004.pdf</fulltext_pdf>
	<start_page>1085</start_page>
	<end_page>1096</end_page>
	<publication_date>2004-07-08</publication_date>
	<article_title content_type="html">Secondary maxima in ozone profiles</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>R. Lemoine</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Royal Meteorological Institute of Belgium, 3, Avenue Circulaire, 1180 Brussels, Belgium</affiliation>
	</affiliations>
	<abstract content_type="html">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.</abstract>
	<references>
	</references>
</article>

