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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>2</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2002</publication_year>
	</journal>
	<doi>10.5194/acpd-2-943-2002</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/2/943/2002/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/2/943/2002/acpd-2-943-2002.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/2/943/2002/acpd-2-943-2002.pdf</fulltext_pdf>
	<start_page>943</start_page>
	<end_page>981</end_page>
	<publication_date>2002-07-10</publication_date>
	<article_title content_type="html">On the origin of tropospheric O&lt;sub&gt;3&lt;/sub&gt; over the Indian Ocean during the winter monsoon: African biomass burning vs. stratosphere-troposphere exchange</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>A. T. J. de Laat</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Space Research Organization Netherlands (SRON), the Netherlands</affiliation>
	</affiliations>
	<abstract content_type="html">A comparison and analysis of modeled and measured
      O&lt;sub&gt;3&lt;/sub&gt; profiles from the INDOEX campaign is presented. European Centre for Medium-Range Weather Forecast&amp;nbsp;
      (ECMWF) meteorological analyses have been assimilated into the model to represent
      actual meteorology. The focus of this study is on two commonly observed features in
      the O&lt;sub&gt;3&lt;/sub&gt;
      profiles: mid tropospheric O&lt;sub&gt;3
      &lt;/sub&gt;maxima (300--500 hPa) over the tropical Indian
      Ocean, and the upper-tropospheric O&lt;sub&gt;3&amp;nbsp;&lt;/sub&gt;
      laminae that occur above approximately 14 km (&amp;gt;150 hPa) altitude. A comparison of model simulated
      O&lt;sub&gt;3&lt;/sub&gt;
      profiles with measured O&lt;sub&gt;3&lt;/sub&gt;
      profiles indicates that the model realistically simulates the observed
      mid-tropospheric O&lt;sub&gt;3&lt;/sub&gt;
      maxima. An analysis of the model simulations shows that the major source of the
      mid-tropospheric O&lt;sub&gt;3&lt;/sub&gt;
      maxima is advection of polluted air masses from continental biomass burning areas over Africa, with generally only a small contribution of
      stratospheric O&lt;sub&gt;3&lt;/sub&gt;. Previous studies hinted at Stratosphere-Troposphere exchange (STE)
      along the subtropical jet (STJ) as the primary source of the mid-tropospheric
      O&lt;sub&gt;3&lt;/sub&gt;
      maxima over the Indian Ocean.&lt;br&gt;
      &lt;br&gt;
      Analysis of the model simulations shows that the mechanism causing the
      mid-tropospheric transport of African biomass burning pollution and stratospheric air
      masses are frontal zones or waves passing along the subtropical jets, causing
      advection of tropical air masses in the prefrontal zone. Furthermore, these frontal
      zones or waves also cause STE at the mid-latitudinal side of the STJ. The model
      simulations also indicate that the contribution of STE in general is minor compared to
      advection and in situ tropospheric production of O&lt;sub&gt;3&lt;/sub&gt;
      for the mid-tropospheric O&lt;sub&gt;3&lt;/sub&gt;
      budget over the Indian Ocean region.&lt;br&gt;
      &lt;br&gt;
      An analysis of the model simulations shows that the model cannot exactly reproduce the measured
      upper-tropospheric O&lt;sub&gt;3
      &lt;/sub&gt;maxima. However, modeled
      O&lt;sub&gt;3
      &lt;/sub&gt;mixing ratios at 14 and
      16 km altitude are significantly higher than at 8 to 12 km altitude, indicating that the model does simulate an upper-tropospheric layer.
      According to the model simulations, the sources of O&lt;sub&gt;3&lt;/sub&gt;
      at 14 and 16 km altitude are advection of both tropospheric and stratospheric
      O&lt;sub&gt;3&lt;/sub&gt;
      as well as in situ O&lt;sub&gt;3&lt;/sub&gt;
      formation.</abstract>
	<references>
	</references>
</article>

