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<!DOCTYPE article SYSTEM "http://www.atmos-chem-phys-discuss.net/inc/acpd/copernicus.dtd">
<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>4</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/acpd-5-6041-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/6041/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/6041/2005/acpd-5-6041-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/6041/2005/acpd-5-6041-2005.pdf</fulltext_pdf>
	<start_page>6041</start_page>
	<end_page>6076</end_page>
	<publication_date>2005-08-17</publication_date>
	<article_title content_type="html">Atmospheric oxidation in the Mexico City Metropolitan Area (MCMA) during April 2003</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>T. R. Shirley</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>W. H. Brune</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>X. Ren</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>J. Mao</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>R. Lesher</name>
		</author>
		<author numeration="6" affiliations="2">
			<name>B. Cardenas</name>
		</author>
		<author numeration="7" affiliations="3">
			<name>R. Volkamer</name>
		</author>
		<author numeration="8" affiliations="3">
			<name>L. T. Molina</name>
		</author>
		<author numeration="9" affiliations="3">
			<name>M. J. Molina</name>
		</author>
		<author numeration="10" affiliations="4">
			<name>B. Lamb</name>
		</author>
		<author numeration="11" affiliations="4">
			<name>E. Velasco</name>
		</author>
		<author numeration="12" affiliations="5">
			<name>T. Jobson</name>
		</author>
		<author numeration="13" affiliations="5">
			<name>M. Alexander</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Dept. of Meteorology, Pennsylvania State University, University Park, Pennsylvania, USA</affiliation>
		<affiliation numeration="2" content_type="html">General Direction of the National Center for Environmental Research and Training (CENICA), National Institute of Ecology (INE), Mexico City, Mexico</affiliation>
		<affiliation numeration="3" content_type="html">Dept. of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts, USA</affiliation>
		<affiliation numeration="4" content_type="html">Dept. of Civil and Environmental Engineering, Washington State University, Pullman, Washington, USA</affiliation>
		<affiliation numeration="5" content_type="html">Atmospheric Sciences, Pacific Northwest National Laboratory, Richland, Washington, USA</affiliation>
	</affiliations>
	<abstract content_type="html">The Mexico City Metropolitan Area (MCMA) study in April 2003 had
measurements of most atmospheric constituents including OH and HO&lt;sub&gt;2&lt;/sub&gt;. It
provided a unique opportunity to examine atmospheric oxidation in a megacity
that has more pollution than typical US and European cities. OH typically
reached 0.35 pptv (~7&amp;times;10&lt;sup&gt;6&lt;/sup&gt; cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt;), comparable to amounts
observed in US cities, but HO&lt;sub&gt;2&lt;/sub&gt; reached 40 pptv in the early afternoon,
more than observed in most US cities. A steady-state photochemical model
simulated the measured OH and HO&lt;sub&gt;2&lt;/sub&gt; for day and night to within combined
measurement and modeling uncertainties for 2/3 of the results. For OH,
measured = 0.65 (modeled) + 0.026 pptv, with R&lt;sup&gt;2&lt;/sup&gt;=0.80. For HO&lt;sub&gt;2&lt;/sub&gt;,
observed = 0.70 (modeled) + 3.4 pptv, with R&lt;sup&gt;2&lt;/sup&gt;=0.64. Measurements
tended to be higher during night and rush hour; the model was higher by
~30% during midday. With a large median measured OH reactivity of
more than 120 s&lt;sup&gt;&amp;minus;1&lt;/sup&gt; during morning rush hour, median ozone production
from observed HO&lt;sub&gt;2&lt;/sub&gt; reached 50 ppb hr&lt;sup&gt;&amp;minus;1&lt;/sup&gt;; RO&lt;sub&gt;2&lt;/sub&gt; was calculated to
have a similar ozone production rate. For both the HO&lt;sub&gt;2&lt;/sub&gt;/OH ratio and the
ozone production, the measured values have the essentially same dependence
on NO as the modeled values. This similarity is unlike other urban studies
in which the NO-dependence of the measured HO&lt;sub&gt;2&lt;/sub&gt;/OH ratio was much less
than the modeled ratio and the ozone production rate that was calculated
from measured HO&lt;sub&gt;2&lt;/sub&gt; unexpectedly appeared to increase as a function of NO
with no obvious peak.</abstract>
	<references>
	</references>
</article>

