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<article language="en">
	<journal>
		<journal_title>Atmospheric Measurement Techniques Discussions</journal_title>
		<journal_url>www.atmos-meas-tech-discuss.net</journal_url>
		<eissn>1867-8610</eissn>
		<volume_number>3</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2010</publication_year>
	</journal>
	<doi>10.5194/amtd-3-3489-2010</doi>
	<article_url>http://www.atmos-meas-tech-discuss.net/3/3489/2010/</article_url>
	<abstract_html>http://www.atmos-meas-tech-discuss.net/3/3489/2010/amtd-3-3489-2010.html</abstract_html>
	<fulltext_pdf>http://www.atmos-meas-tech-discuss.net/3/3489/2010/amtd-3-3489-2010.pdf</fulltext_pdf>
	<start_page>3489</start_page>
	<end_page>3534</end_page>
	<publication_date>2010-08-18</publication_date>
	<article_title content_type="html">A geostationary thermal infrared sensor to monitor the lowermost troposphere: O&lt;sub&gt;3&lt;/sub&gt; and CO retrieval studies</article_title>
	<authors>
		<author numeration="1" affiliations="1,2">
			<name>M. Claeyman</name>
			<email>marine.claeyman@aero.obs-mip.fr</email>
		</author>
		<author numeration="2" affiliations="1,2">
			<name>J.-L. Attié</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>V.-H. Peuch</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>L. El Amraoui</name>
		</author>
		<author numeration="5" affiliations="2,3">
			<name>W. A. Lahoz</name>
		</author>
		<author numeration="6" affiliations="2">
			<name>B. Josse</name>
		</author>
		<author numeration="7" affiliations="1">
			<name>P. Ricaud</name>
		</author>
		<author numeration="8" affiliations="4">
			<name>T. von Clarmann</name>
		</author>
		<author numeration="9" affiliations="4">
			<name>M. Höpfner</name>
		</author>
		<author numeration="10" affiliations="4">
			<name>J. Orphal</name>
		</author>
		<author numeration="11" affiliations="5">
			<name>J.-M. Flaud</name>
		</author>
		<author numeration="12" affiliations="6">
			<name>D. P. Edwards</name>
		</author>
		<author numeration="13" affiliations="7">
			<name>K. Chance</name>
		</author>
		<author numeration="14" affiliations="7">
			<name>X. Liu</name>
		</author>
		<author numeration="15" affiliations="8">
			<name>F. Pasternak</name>
		</author>
		<author numeration="16" affiliations="8">
			<name>R. Cantié</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Laboratoire d&apos;Aérologie, Université de Toulouse, CNRS/INSU, Toulouse, France</affiliation>
		<affiliation numeration="2" content_type="html">CNRM-GAME, Météo-France and CNRS URA 1357, Toulouse, France</affiliation>
		<affiliation numeration="3" content_type="html">NILU, N-2027 Kjeller, Norway</affiliation>
		<affiliation numeration="4" content_type="html">Karlsruhe Institute of Technology, IMK, Karlsruhe, Germany</affiliation>
		<affiliation numeration="5" content_type="html">Laboratoire Interuniversitaire des Systèmes Atmosphériques, CNRS UMR 7583, Université de Paris-Est, Créteil, France</affiliation>
		<affiliation numeration="6" content_type="html">National Center for Atmospheric Research, Boulder, Colorado, USA</affiliation>
		<affiliation numeration="7" content_type="html">Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA</affiliation>
		<affiliation numeration="8" content_type="html">Astrium-EADS, Toulouse, France</affiliation>
	</affiliations>
	<abstract content_type="html">This paper describes the capabilities of a nadir thermal infrared (TIR)
sensor proposed for embarkation onboard a geostationary platform to monitor
ozone (O&lt;sub&gt;3&lt;/sub&gt;) and carbon monoxide (CO) for air quality (AQ) purposes. To
assess the capabilities of this sensor we perform idealized retrieval studies
considering typical atmospheric profiles of O&lt;sub&gt;3&lt;/sub&gt; and CO over Europe with
different instrument configurations (signal to noise ratio and spectral
sampling interval) using the KOPRA forward model and the KOPRA-fit retrieval
scheme based on the Tikhonov-Phillips regularization. We then select a
configuration, referred to as GEO-TIR, optimized for providing information in
the lowermost troposphere (LmT; 0–3 km in height). For the GEO-TIR
configuration we obtain around 1.5 degrees of freedom for O&lt;sub&gt;3&lt;/sub&gt; and 2 for CO
at altitudes between 0 and 15 km. The error budget of GEO-TIR, calculated
taking account of the principal contributions to the error (namely,
temperature, measurement error, smoothing error) shows that information in
the LmT can be achieved by GEO-TIR. We also retrieve analogous profiles from
another geostationary infrared instrument with characteristics similar to the
Meteosat Third Generation Infrared Sounder (MTG-IRS) which is dedicated to
numerical weather prediction, referred to as GEO-TIR2. Comparison between
GEO-TIR and GEO-TIR2 allows us to quantify the added value of GEO-TIR, a
mission complementing the AQ observing system. To better characterize the
information provided by GEO-TIR and GEO-TIR2 in the LmT, we retrieve two
typical profiles of O&lt;sub&gt;3&lt;/sub&gt; and CO for different thermal contrast ranging from
–10 K to 10 K. The shape of the first averaging kernel (corresponding to
the surface level) confirms that GEO-TIR has good sensitivity to CO in the
LmT and also to O&lt;sub&gt;3&lt;/sub&gt; for high positive thermal contrast. GEO-TIR2 has very
low sensitivity in the LmT to O&lt;sub&gt;3&lt;/sub&gt; but can have sensitivity to CO with high
positive thermal contrast. To quantify these results for a realistic
atmosphere, we simulate it using the chemical transport model MOCAGE
(MOdèle de Chimie Atmospherique à Grande Echelle) – this is the
nature run. We simulate the O&lt;sub&gt;3&lt;/sub&gt; and CO spatial and temporal distributions
from GEO-TIR observations in the LmT in July 2009 over Europe by sampling the
nature run. Results show that GEO-TIR is able to capture well the
spatial and temporal variability in the LmT for both O&lt;sub&gt;3&lt;/sub&gt; and CO,
particularly during periods with high positive thermal contrast near the
ground and high surface temperature, which results in active photochemistry
and a raised planetary boundary layer. These results also provide evidence of
the significant added value in the LmT of GEO-TIR compared to GEO-TIR2 by
showing GEO-TIR is closer to the nature run than GEO-TIR2 for various
statistical parameters (correlation, bias, standard deviation).</abstract>
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</article>

