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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>6</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/acpd-5-12031-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/12031/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/12031/2005/acpd-5-12031-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/12031/2005/acpd-5-12031-2005.pdf</fulltext_pdf>
	<start_page>12031</start_page>
	<end_page>12066</end_page>
	<publication_date>2005-11-23</publication_date>
	<article_title content_type="html">Retrieval of stratospheric ozone profiles from MIPAS/ENVISAT limb emission spectra: a sensitivity study</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>N. Glatthor</name>
			<email>norbert.glatthor@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="2">
			<name>S. Gil-López</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>A. Linden</name>
		</author>
		<author numeration="10" affiliations="2">
			<name>M. López-Puertas</name>
		</author>
		<author numeration="11" affiliations="1,3">
			<name>G. Mengistu Tsidu</name>
		</author>
		<author numeration="12" affiliations="1">
			<name>M. Milz</name>
		</author>
		<author numeration="13" affiliations="1">
			<name>T. Steck</name>
		</author>
		<author numeration="14" affiliations="1">
			<name>G. P. Stiller</name>
		</author>
		<author numeration="15" affiliations="1,4">
			<name>D.-Y. Wang</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Forschungszentrum Karlsruhe, Institut für Meteorologie und Klimaforschung, Karlsruhe, Germany</affiliation>
		<affiliation numeration="2" content_type="html">Instituto de Astrof&amp;iacute;sica de Andaluc&amp;iacute;a (CSIC), Granada, Spain</affiliation>
		<affiliation numeration="3" content_type="html">now at: Universität Bremen, Fachbereich Physik/Elektrotechnik, Institut für Umweltphysik, Bremen, Germany</affiliation>
		<affiliation numeration="4" content_type="html">now at: SAIC/GSO: MODIS Characterization Support Team, Seabrook, MD 20706, USA</affiliation>
	</affiliations>
	<abstract content_type="html">We report on the dependance of ozone volume mixing ratio profiles, retrieved from spectra of the Michelson
Interferometer for Passive Atmospheric Sounding (MIPAS), on different retrieval setups such as
different a-priori profiles, regularization strengths and spectral regions used for analysis.
MIPAS is a spaceborne limb-viewing Fourier transform infrared (FTIR) emission spectrometer,
by which vertical profiles of various trace gases can be measured simultaneously.
Purpose of this investigation is to check and to optimize the current retrieval setup.
The choice of different a-priori profiles, of a different approach to retrieve the continuum
radiation, and of a weaker regularization than in the reference data version (V2_O3_2)
causes only small to moderate deviations of up to &amp;plusmn;0.2, &amp;minus;0.3 and &amp;plusmn;0.5 ppmv,
respectively, in the retrieved ozone volume mixing ratios below 60 km altitude. Use of
different microwindow sets optimized for polar, mid-latitude and tropical conditions results
in deviations of up to &amp;plusmn;1.5 ppmv in the altitude region of the ozone maximum, exceeding
the total estimated retrieval error of 0.65 ppmv (polar regions) &amp;ndash; 1.2 ppmv (tropics) in
this height region. Therefore, to avoid latitudinal artefacts,
one fixed set of microwindows is considered more appropriate for retrieval of a whole orbit rather
than a latitude-dependent microwindow selection. For this task the microwindow set optimized for the
polar atmosphere was found to be better suitable than its midlatitude and tropical
counterparts.
The results from the different microwindow sets, which variably cover MIPAS spectral
bands A (685&amp;ndash;970 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt;) and AB (1020&amp;ndash;1170 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt;), indicated a positive bias of up
to 1ppmv between the ozone maxima retrieved from the ozone emission in MIPAS band AB
only and from combined analysis of MIPAS bands A and AB. Further investigations showed
that this discrepancy can be caused by a bias between the radiance calibration
of level-1B spectra of bands A and AB or by a bias between the spectroscopic
data used in bands A and AB.</abstract>
	<references>
	</references>
</article>

