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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>7</volume_number>
		<issue_number>2</issue_number>
		<publication_year>2007</publication_year>
	</journal>
	<doi>10.5194/acpd-7-3333-2007</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/7/3333/2007/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/7/3333/2007/acpd-7-3333-2007.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/7/3333/2007/acpd-7-3333-2007.pdf</fulltext_pdf>
	<start_page>3333</start_page>
	<end_page>3395</end_page>
	<publication_date>2007-03-02</publication_date>
	<article_title content_type="html">Validation of MIPAS-ENVISAT NO&lt;sub&gt;2&lt;/sub&gt; operational data</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>G. Wetzel</name>
			<email>gerald.wetzel@imk.fzk.de</email>
		</author>
		<author numeration="2" affiliations="2">
			<name>A. Bracher</name>
		</author>
		<author numeration="3" affiliations="3">
			<name>B. Funke</name>
		</author>
		<author numeration="4" affiliations="4">
			<name>F. Goutail</name>
		</author>
		<author numeration="5" affiliations="5">
			<name>F. Hendrick</name>
		</author>
		<author numeration="6" affiliations="5">
			<name>J.-C. Lambert</name>
		</author>
		<author numeration="7" affiliations="1">
			<name>S. Mikuteit</name>
		</author>
		<author numeration="8" affiliations="6">
			<name>C. Piccolo</name>
		</author>
		<author numeration="9" affiliations="7">
			<name>M. Pirre</name>
		</author>
		<author numeration="10" affiliations="4">
			<name>A. Bazureau</name>
		</author>
		<author numeration="11" affiliations="8">
			<name>C. Belotti</name>
		</author>
		<author numeration="12" affiliations="1">
			<name>T. Blumenstock</name>
		</author>
		<author numeration="13" affiliations="5">
			<name>M. De Mazière</name>
		</author>
		<author numeration="14" affiliations="1">
			<name>H. Fischer</name>
		</author>
		<author numeration="15" affiliations="7">
			<name>N. Huret</name>
		</author>
		<author numeration="16" affiliations="4">
			<name>D. Ionov</name>
		</author>
		<author numeration="17" affiliations="3">
			<name>M. López-Puertas</name>
		</author>
		<author numeration="18" affiliations="1">
			<name>G. Maucher</name>
		</author>
		<author numeration="19" affiliations="1">
			<name>H. Oelhaf</name>
		</author>
		<author numeration="20" affiliations="4">
			<name>J.-P. Pommereau</name>
		</author>
		<author numeration="21" affiliations="1">
			<name>R. Ruhnke</name>
		</author>
		<author numeration="22" affiliations="2">
			<name>M. Sinnhuber</name>
		</author>
		<author numeration="23" affiliations="1">
			<name>G. Stiller</name>
		</author>
		<author numeration="24" affiliations="5">
			<name>M. Van Roozendael</name>
		</author>
		<author numeration="25" affiliations="1,9">
			<name>G. Zhang</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institut für Meteorologie und Klimaforschung (IMK), Forschungszentrum Karlsruhe, Karlsruhe, Germany</affiliation>
		<affiliation numeration="2" content_type="html">Institute of Environmental Physics and Remote Sensing (IUP/IFE), University of Bremen, Bremen, Germany</affiliation>
		<affiliation numeration="3" content_type="html">Instituto de Astrofísica de Andalucía (IAA), Consejo Superior de Investigaciones Cientificas, Granada, Spain</affiliation>
		<affiliation numeration="4" content_type="html">Service d&apos;Aéronomie, CNRS, Verrières-le-Buisson, France</affiliation>
		<affiliation numeration="5" content_type="html">Belgian Institute for Space Aeronomy (IASB-BIRA), Brussels, Belgium</affiliation>
		<affiliation numeration="6" content_type="html">Oxford University, Oxford, UK</affiliation>
		<affiliation numeration="7" content_type="html">Laboratoire de Physique et Chimie de l&apos;Environnement (LPCE), CNRS, Orléans, France</affiliation>
		<affiliation numeration="8" content_type="html">IFAC-CNR, Firenze, Italy</affiliation>
		<affiliation numeration="9" content_type="html">now at: Yantai University, Yantai, China</affiliation>
	</affiliations>
	<abstract content_type="html">The Michelson Interferometer for Passive Atmospheric Sounding (MIPAS)
instrument was launched aboard the environmental satellite ENVISAT into its
sun-synchronous orbit on 1 March 2002. The short-lived species NO&lt;sub&gt;2&lt;/sub&gt; is
one of the key target products of MIPAS that are operationally retrieved
from limb emission spectra measured in the stratosphere and mesosphere.
Within the MIPAS validation activities, a large number of independent
observations from balloons, satellites and ground-based stations have been
compared to European Space Agency (ESA) version 4.61 operational NO&lt;sub&gt;2&lt;/sub&gt;
data comprising the time period from July 2002 until March 2004 where MIPAS
measured with full spectral resolution. Comparisons between MIPAS and
balloon-borne observations carried out in 2002 and 2003 in the Arctic, at
mid-latitudes, and in the tropics show a very good agreement below 40 km
altitude with a mean deviation of roughly 3%, virtually without any
significant bias. The comparison to ACE satellite observations exhibits only
a small negative bias of MIPAS which appears not to be significant. The
independent satellite instruments HALOE, SAGE II, and POAM III confirm in
common for the spring-summer time period a negative bias of MIPAS in the
Arctic and a positive bias in the Antarctic middle and upper stratosphere
exceeding frequently the combined systematic error limits. In contrast to
the ESA operational processor, the IMK/IAA retrieval code allows accurate
inference of NO&lt;sub&gt;2&lt;/sub&gt; volume mixing ratios under consideration of all
important non-LTE processes. Large differences between both retrieval
results appear especially at higher altitudes, above about 50 to 55 km.
These differences might be explained at least partly by non-LTE under polar
winter conditions but not at mid-latitudes. Below this altitude region mean
differences between both processors remain within 5% (during night) and
up to 10% (during day) under undisturbed (September 2002) conditions and
up to 40% under perturbed polar night conditions (February and March
2004). The intercomparison of ground-based NDACC observations shows no
significant bias between the FTIR measurements in Kiruna (68&amp;deg; N) and
MIPAS in summer 2003 but larger deviations in autumn and winter. The mean
deviation over the whole comparison period remains within 10%. A mean
negative bias of 15% for MIPAS daytime and 8% for nighttime
observations has been determined for UV-vis comparisons over Harestua (60&amp;deg; N).
Results of a pole-to-pole comparison of ground-based DOAS/UV-visible
sunrise and MIPAS mid-morning column data has shown that the mean agreement
in 2003 falls within the accuracy limit of the comparison method.
Altogether, it can be indicated that MIPAS NO&lt;sub&gt;2&lt;/sub&gt; profiles yield valuable
information on the vertical distribution of NO&lt;sub&gt;2&lt;/sub&gt; in the lower and middle
stratosphere (below about 45 km) during day and night with an overall
accuracy of about 10&amp;ndash;20% and a precision of typically 5&amp;ndash;15% such that
the data are useful for scientific studies. In cases where extremely high
NO&lt;sub&gt;2&lt;/sub&gt; occurs in the mesosphere (polar winter) retrieval results in the
lower and middle stratosphere are less accurate than under undisturbed
atmospheric conditions.</abstract>
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</article>

