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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>5</volume_number>
		<issue_number>3</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/acpd-5-3747-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/3747/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/3747/2005/acpd-5-3747-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/3747/2005/acpd-5-3747-2005.pdf</fulltext_pdf>
	<start_page>3747</start_page>
	<end_page>3771</end_page>
	<publication_date>2005-06-07</publication_date>
	<article_title content_type="html">Influence of convective transport on tropospheric ozone and its precursors in a chemistry-climate model</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>R. M. Doherty</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>D. S. Stevenson</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>W. J. Collins</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>M. G. Sanderson</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institute of Atmospheric and Environmental Science, University of Edinburgh, Edinburgh, UK</affiliation>
		<affiliation numeration="2" content_type="html">Hadley Centre for Climate Prediction and Research, Met Office, Exeter, UK</affiliation>
	</affiliations>
	<abstract content_type="html">The impact of convection on tropospheric O&lt;sub&gt;3&lt;/sub&gt; and its precursors has been
examined in a coupled chemistry-climate model. There are two ways that
convection affects O&lt;sub&gt;3&lt;/sub&gt;. First, convection affects O&lt;sub&gt;3&lt;/sub&gt; by vertical
mixing of O&lt;sub&gt;3&lt;/sub&gt; itself. Convection lifts lower tropospheric air to regions
where the ozone lifetime is longer, whilst mass-balance subsidence mixes
O&lt;sub&gt;3&lt;/sub&gt;-rich upper tropospheric (UT) air downwards to regions where the
O&lt;sub&gt;3&lt;/sub&gt; lifetime is shorter. This tends to decrease UT ozone and the overall
tropospheric column of O&lt;sub&gt;3&lt;/sub&gt;. Secondly, convection affects O&lt;sub&gt;3&lt;/sub&gt; by
vertical mixing of ozone precursors. This affects O&lt;sub&gt;3&lt;/sub&gt; chemical
production and destruction. Convection transports isoprene and its
degradation products to the UT where they interact with lightning NO&lt;sub&gt;x&lt;/sub&gt;
to produce PAN, at the expense of NO&lt;sub&gt;x&lt;/sub&gt;. The combined effect of NO&lt;sub&gt;x&lt;/sub&gt;
to PAN conversions and downward transport of lightning NO&lt;sub&gt;x&lt;/sub&gt; results in
UT NO&lt;sub&gt;x&lt;/sub&gt; decreases. Convective lofting of NO&lt;sub&gt;x&lt;/sub&gt; from surface sources
appears relatively unimportant. Despite UT NO&lt;sub&gt;x&lt;/sub&gt; decreases, UT O&lt;sub&gt;3&lt;/sub&gt; production increases as a result of UT HO&lt;sub&gt;x&lt;/sub&gt; increases driven by isoprene
oxidation chemistry. However, UT O&lt;sub&gt;3&lt;/sub&gt; tends to decrease, as the effect of
convective overturning of O&lt;sub&gt;3&lt;/sub&gt; itself dominates over changes in O&lt;sub&gt;3&lt;/sub&gt; chemistry. The changes in tropical UT O&lt;sub&gt;3&lt;/sub&gt; are transported polewards
resulting in a 15% decrease in the global tropospheric O&lt;sub&gt;3&lt;/sub&gt; burden.
These results contrast with an earlier study that uses a model of similar
chemical complexity. Differences in chemistry schemes - in particular
isoprene-driven changes, as well as differences in convection schemes
themselves, are the most likely causes of such discrepancies. Further
modelling studies are needed to constrain this uncertainty range.</abstract>
	<references>
	</references>
</article>

