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<article language="en">
	<journal>
		<journal_title>Atmospheric Chemistry and Physics</journal_title>
		<journal_url>www.atmos-chem-phys.net</journal_url>
		<issn>1680-7316</issn>
		<eissn>1680-7324</eissn>
		<volume_number>7</volume_number>
		<issue_number>13</issue_number>
		<publication_year>2007</publication_year>
	</journal>
	<doi>10.5194/acp-7-3639-2007</doi>
	<article_url>http://www.atmos-chem-phys.net/7/3639/2007/</article_url>
	<abstract_html>http://www.atmos-chem-phys.net/7/3639/2007/acp-7-3639-2007.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys.net/7/3639/2007/acp-7-3639-2007.pdf</fulltext_pdf>
	<start_page>3639</start_page>
	<end_page>3662</end_page>
	<publication_date>2007-07-11</publication_date>
	<article_title content_type="html">Bias determination and precision validation of ozone profiles from MIPAS-Envisat retrieved with the IMK-IAA processor</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>T. Steck</name>
			<email>tilman.steck@imk.fzk.de</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>T. von Clarmann</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>H. Fischer</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>B. Funke</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>N. Glatthor</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>U. Grabowski</name>
		</author>
		<author numeration="7" affiliations="1">
			<name>M. Höpfner</name>
		</author>
		<author numeration="8" affiliations="1">
			<name>S. Kellmann</name>
		</author>
		<author numeration="9" affiliations="1">
			<name>M. Kiefer</name>
		</author>
		<author numeration="10" affiliations="1">
			<name>A. Linden</name>
		</author>
		<author numeration="11" affiliations="1">
			<name>M. Milz</name>
		</author>
		<author numeration="12" affiliations="1">
			<name>G. P. Stiller</name>
		</author>
		<author numeration="13" affiliations="3">
			<name>D. Y. Wang</name>
		</author>
		<author numeration="14" affiliations="4">
			<name>M. Allaart</name>
		</author>
		<author numeration="15" affiliations="1">
			<name>Th. Blumenstock</name>
		</author>
		<author numeration="16" affiliations="5">
			<name>P. von der Gathen</name>
		</author>
		<author numeration="17" affiliations="6">
			<name>G. Hansen</name>
		</author>
		<author numeration="18" affiliations="1">
			<name>F. Hase</name>
		</author>
		<author numeration="19" affiliations="1">
			<name>G. Hochschild</name>
		</author>
		<author numeration="20" affiliations="1">
			<name>G. Kopp</name>
		</author>
		<author numeration="21" affiliations="7">
			<name>E. Kyrö</name>
		</author>
		<author numeration="22" affiliations="1">
			<name>H. Oelhaf</name>
		</author>
		<author numeration="23" affiliations="8">
			<name>U. Raffalski</name>
		</author>
		<author numeration="24" affiliations="9">
			<name>A. Redondas Marrero</name>
		</author>
		<author numeration="25" affiliations="10">
			<name>E. Remsberg</name>
		</author>
		<author numeration="26" affiliations="11">
			<name>J. Russell III</name>
		</author>
		<author numeration="27" affiliations="6">
			<name>K. Stebel</name>
		</author>
		<author numeration="28" affiliations="12">
			<name>W. Steinbrecht</name>
		</author>
		<author numeration="29" affiliations="1">
			<name>G. Wetzel</name>
		</author>
		<author numeration="30" affiliations="13">
			<name>M. Yela</name>
		</author>
		<author numeration="31" affiliations="1">
			<name>G. Zhang</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institut für Meteorologie und Klimaforschung, Forschungszentrum Karlsruhe, Germany</affiliation>
		<affiliation numeration="2" content_type="html">Instituto de Astrofísica de Andalucía, Granada, Spain</affiliation>
		<affiliation numeration="3" content_type="html">Physics Department, University of New Brunswick, Canada</affiliation>
		<affiliation numeration="4" content_type="html">KNMI (Royal Netherlands Meteorological Institute), De Bilt, The Netherlands</affiliation>
		<affiliation numeration="5" content_type="html">Alfred Wegener Institute for Polar and Marine Research, Potsdam, Germany</affiliation>
		<affiliation numeration="6" content_type="html">Norwegian Institute for Air Research (NILU), Polar Environmental Centre, Tromsø, Norway</affiliation>
		<affiliation numeration="7" content_type="html">FMI-Arctic Research Centre, Sodankylä, Finland</affiliation>
		<affiliation numeration="8" content_type="html">Swedish Institute of Space Physics (IRF), Kiruna, Sweden</affiliation>
		<affiliation numeration="9" content_type="html">Instituto Nacional de Meteorologia (INM), Santa Cruz de Tenerife, Spain</affiliation>
		<affiliation numeration="10" content_type="html">Atmospheric Sciences Competency, NASA Langley Research Center, Hampton, USA</affiliation>
		<affiliation numeration="11" content_type="html">Department of Physics, Hampton University, Hampton, USA</affiliation>
		<affiliation numeration="12" content_type="html">Deutscher Wetterdienst (DWD), Hohenpeißenberg, Germany</affiliation>
		<affiliation numeration="13" content_type="html">Instituto Nacional de Técnica Aeroespacial (INTA), Torrejón de Ardoz, Spain</affiliation>
	</affiliations>
	<abstract content_type="html">This paper characterizes vertical ozone profiles retrieved with the IMK-IAA
(Institute for Meteorology and Climate Research, Karlsruhe &amp;ndash; Instituto de
Astrofisica de Andalucia) science-oriented processor from high spectral
resolution data (until March 2004) measured by the Michelson Interferometer
for Passive Atmospheric Sounding (MIPAS) aboard the environmental satellite
Envisat. Bias determination and precision validation is performed on the
basis of correlative
measurements by ground-based lidars, Fourier transform infrared spectrometers,
and microwave radiometers as well as balloon-borne ozonesondes, the
balloon-borne version of MIPAS, and two satellite instruments (Halogen
Occultation Experiment and Polar Ozone and Aerosol Measurement III).
Percentage mean differences between MIPAS and the comparison instruments for
stratospheric ozone are generally within &amp;plusmn;10%. The precision in this
altitude region is estimated at values between 5 and 10% which gives an
accuracy of 15 to 20%.
Below 18 km, the spread of the percentage mean differences is larger and
the precision degrades to values of more than 20% depending on altitude
and latitude. The main reason for the degraded precision at low altitudes is
attributed
to undetected thin clouds which affect MIPAS retrievals, and to the
influence of uncertainties in the water vapor concentration.</abstract>
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</article>

