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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>9</volume_number>
		<issue_number>3</issue_number>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/acpd-9-11551-2009</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/9/11551/2009/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/9/11551/2009/acpd-9-11551-2009.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/9/11551/2009/acpd-9-11551-2009.pdf</fulltext_pdf>
	<start_page>11551</start_page>
	<end_page>11587</end_page>
	<publication_date>2009-05-11</publication_date>
	<article_title content_type="html">First multi-year occultation observations of CO&lt;sub&gt;2&lt;/sub&gt; in the MLT by ACE satellite: observations and analysis using the extended CMAM</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>S. R. Beagley</name>
			<email>beagley@nimbus.yorku.ca</email>
		</author>
		<author numeration="2" affiliations="2">
			<name>C. D. Boone</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>V. I. Fomichev</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>J. J. Jin</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>K. Semeniuk</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>J. C. McConnell</name>
		</author>
		<author numeration="7" affiliations="2,3">
			<name>P. F. Bernath</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Department of Earth and Space Science and Engineering, York University, Toronto, Ontario, Canada</affiliation>
		<affiliation numeration="2" content_type="html">Department of Chemistry, University of Waterloo, Waterloo, Ontario, Canada</affiliation>
		<affiliation numeration="3" content_type="html">Department of Chemistry, University of York, Heslington, York, UK</affiliation>
	</affiliations>
	<abstract content_type="html">This paper presents the first multi-year global set of observations of
CO&lt;sub&gt;2&lt;/sub&gt; in the mesosphere and lower thermosphere (MLT) obtained by the
ACE-FTS instrument on SCISAT-I, a small Canadian satellite launched in 2003.
The observations use the solar occultation technique and document the
fall-off in the mixing ratio of CO&lt;sub&gt;2&lt;/sub&gt; in the MLT region. The beginning of
the fall-off of the CO&lt;sub&gt;2&lt;/sub&gt;, or &quot;knee&quot; occurs at about 78 km and lies
higher than in the CRISTA measurements (~70 km) but lower than in the
SABER 1.06 (~82 km) and much lower than in rocket measurements. We
also present the measurements of CO obtained concurrently which provide
important constraints for analysis. We have compared the ACE measurements
with simulations of the CO&lt;sub&gt;2&lt;/sub&gt; and CO distributions in the vertically
extended version of the Canadian Middle Atmosphere Model (CMAM). Applying
standard chemistry we find that we cannot get agreement between the model
and ACE CO&lt;sub&gt;2&lt;/sub&gt; observations although the CO observations are adequately
reproduced. There appears to be about a 10 km offset compared to the
observed ACE CO&lt;sub&gt;2&lt;/sub&gt;, with the model knee occurring too high. In analysing
the disagreement, we have investigated the variation of several parameters
of interest, photolysis rates, formation rate for CO&lt;sub&gt;2&lt;/sub&gt;, and the impact
of uncertainty in eddy diffusion, in order to explore parameter space for
this problem. Our conclusions are that there must be a loss process for
CO&lt;sub&gt;2&lt;/sub&gt;, about 2–4 times faster than photolysis that will sequester the
carbon in some form other than CO and we have speculated on the role of
meteoritic dust as a possible candidate. In addition, from this study we
have highlighted a possible important role for vertical eddy diffusion in 3-D
models in determining the distribution of candidate species in the
mesosphere which requires further study.</abstract>
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</article>

