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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>6</volume_number>
		<issue_number>6</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acpd-6-11465-2006</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/6/11465/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/6/11465/2006/acpd-6-11465-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/6/11465/2006/acpd-6-11465-2006.pdf</fulltext_pdf>
	<start_page>11465</start_page>
	<end_page>11520</end_page>
	<publication_date>2006-11-17</publication_date>
	<article_title content_type="html">Remote sensed and in situ constraints on processes affecting tropical tropospheric ozone</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>B. Sauvage</name>
		</author>
		<author numeration="2" affiliations="1,2">
			<name>R. V. Martin</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>A. van Donkelaar</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>X. Liu</name>
		</author>
		<author numeration="5" affiliations="2">
			<name>K. Chance</name>
		</author>
		<author numeration="6" affiliations="3">
			<name>L. Jaeglé</name>
		</author>
		<author numeration="7" affiliations="4">
			<name>P. I. Palmer</name>
		</author>
		<author numeration="8" affiliations="5">
			<name>S. Wu</name>
		</author>
		<author numeration="9" affiliations="5">
			<name>T.-M. Fu</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Department of Physics and Atmospheric Science, Dalhousie University, Halifax, Nova Scotia, Canada</affiliation>
		<affiliation numeration="2" content_type="html">Atomic and Molecular Physics Division, Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts, USA</affiliation>
		<affiliation numeration="3" content_type="html">Department of Atmospheric Sciences, University of Washington, Seattle, Washington, USA</affiliation>
		<affiliation numeration="4" content_type="html">School of GeoSciences, University of Edinburgh, UK</affiliation>
		<affiliation numeration="5" content_type="html">Department of Earth and Planetary Sciences and Division of Engineering and Applied Sciences, Harvard University, Cambridge, Massachusetts, USA</affiliation>
	</affiliations>
	<abstract content_type="html">We use a global chemical transport model (GEOS-Chem)
to evaluate the consistency of satellite
measurements of lightning flashes and ozone
precursors with in situ measurements of
tropical tropospheric ozone. The measurements
are tropospheric O&lt;sub&gt;3&lt;/sub&gt;, NO&lt;sub&gt;2&lt;/sub&gt;, and HCHO columns from the GOME satellite
instrument, lightning flashes from the OTD and LIS instruments,
profiles of O&lt;sub&gt;3&lt;/sub&gt;, CO, and relative humidity from the MOZAIC
aircraft program, and profiles of O&lt;sub&gt;3&lt;/sub&gt; from the SHADOZ ozonesonde
network. We interpret these multiple
data sources with our
model to better understand what controls tropical
tropospheric ozone. Tropical tropospheric ozone is mainly affected
by lightning and convection in the upper troposphere and
by surface emissions in the lower troposphere.
Scaling the spatial
distribution of lightning in the model to the observed flash counts improves the
simulation of O&lt;sub&gt;3&lt;/sub&gt; in the upper troposphere by 5&amp;ndash;20&amp;nbsp;ppbv versus
in situ observations and by 1&amp;ndash;4&amp;nbsp;Dobson Units versus GOME retrievals of tropospheric O&lt;sub&gt;3&lt;/sub&gt; columns.
A lightning source strength of 5&amp;plusmn;2&amp;nbsp;Tg N/yr best represents in situ observations from
aircraft and ozonesonde.  Tropospheric NO&lt;sub&gt;2&lt;/sub&gt; and HCHO
columns from GOME are applied to provide top-down constraints on
emission inventories of NO&lt;sub&gt;x&lt;/sub&gt; (biomass burning and soils) and VOCs
(biomass burning). The top-down
biomass burning inventory is larger by a factor of 2 for HCHO and alkenes,
and by 2.6 for NO&lt;sub&gt;x&lt;/sub&gt; over northern equatorial Africa. These emissions increase lower tropospheric O&lt;sub&gt;3&lt;/sub&gt;
by 5&amp;ndash;20&amp;nbsp;ppbv, improving the simulation versus aircraft observations,
and by 4&amp;nbsp;Dobson Units versus
GOME observations of tropospheric O&lt;sub&gt;3&lt;/sub&gt; columns. Emission factors in the a posteriori inventory are more
consistent with a recent compilation from in situ measurements.  The ozone simulation
using two different dynamical schemes (GEOS-3 and GEOS-4) is
evaluated versus observations; GEOS-4 better represents O&lt;sub&gt;3&lt;/sub&gt;
observations by 5&amp;ndash;15&amp;nbsp;ppbv due to enhanced convective detrainment in the
upper troposphere.
Heterogeneous uptake of HNO&lt;sub&gt;3&lt;/sub&gt; on aerosols reduces
simulated O&lt;sub&gt;3&lt;/sub&gt; by 5&amp;ndash;7&amp;nbsp;ppbv, reducing a model bias versus in situ
observations over and downwind of deserts.
Exclusion of HO&lt;sub&gt;2&lt;/sub&gt; uptake on aerosols improves O&lt;sub&gt;3&lt;/sub&gt; by 5&amp;nbsp;ppbv in biomass burning regions.</abstract>
	<references>
	</references>
</article>

