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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>6</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acpd-6-6525-2006</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/6/6525/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/6/6525/2006/acpd-6-6525-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/6/6525/2006/acpd-6-6525-2006.pdf</fulltext_pdf>
	<start_page>6525</start_page>
	<end_page>6585</end_page>
	<publication_date>2006-07-13</publication_date>
	<article_title content_type="html">MIPAS level 2 operational analysis</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>P. Raspollini</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>C. Belotti</name>
		</author>
		<author numeration="3" affiliations="6">
			<name>A. Burgess</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>B. Carli</name>
		</author>
		<author numeration="5" affiliations="2">
			<name>M. Carlotti</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>S. Ceccherini</name>
		</author>
		<author numeration="7" affiliations="3">
			<name>B. M. Dinelli</name>
		</author>
		<author numeration="8" affiliations="6">
			<name>A. Dudhia</name>
		</author>
		<author numeration="9" affiliations="5">
			<name>J.-M. Flaud</name>
		</author>
		<author numeration="10" affiliations="8">
			<name>B. Funke</name>
		</author>
		<author numeration="11" affiliations="4">
			<name>M. Höpfner</name>
		</author>
		<author numeration="12" affiliations="8">
			<name>M. Lopez-Puertas</name>
		</author>
		<author numeration="13" affiliations="6">
			<name>V. Payne</name>
		</author>
		<author numeration="14" affiliations="6">
			<name>C. Piccolo</name>
		</author>
		<author numeration="15" affiliations="7">
			<name>J. J. Remedios</name>
		</author>
		<author numeration="16" affiliations="2">
			<name>M. Ridolfi</name>
		</author>
		<author numeration="17" affiliations="7,9">
			<name>R. Spang</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Istituto di Fisica Applicata “N. Carrara&quot; (IFAC) del Consiglio Nazionale delle Ricerche (CNR), Firenze, Italy</affiliation>
		<affiliation numeration="2" content_type="html">Dipartimento di Chimica Fisica e Inorganica, University of Bologna, Bologna, Italy</affiliation>
		<affiliation numeration="3" content_type="html">Istituto di Scienza dell’Atmosfera e del Clima (ISAC) del Consiglio Nazionale delle Ricerche (CNR), Bologna, Italy</affiliation>
		<affiliation numeration="4" content_type="html">Forschungszentrum Karlsruhe GmbH, Institut für Meteorologie und Klimaforschung, Germany</affiliation>
		<affiliation numeration="5" content_type="html">Laboratoire Interuniversitaire des Systèmes Atmosphériques (LISA) CNRS/ Univ Paris 12 et 7, France</affiliation>
		<affiliation numeration="6" content_type="html">Atmospheric, Oceanic and Planetary Physics – Clarendon Laboratory – Oxford University, UK</affiliation>
		<affiliation numeration="7" content_type="html">Earth Observation Science, Department of Physics and Astronomy, University of Leicester, UK</affiliation>
		<affiliation numeration="8" content_type="html">Instituto de Astrof&amp;#205;sica de Andaluc&amp;#205;a (CSIC), Granada, Spain</affiliation>
		<affiliation numeration="9" content_type="html">now at: ICGI Forschungszentrum Jülich, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">The MIPAS (Michelson Interferometer for Passive Atmospheric Sounding)
instrument has been operating on-board the ENVISAT satellite since March
2002. In the first two years, it acquired in a nearly continuous manner high
resolution (0.025 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt; unapodised) emission spectra of the Earth&apos;s
atmosphere at limb in the middle infrared region. This paper describes the
level&amp;nbsp;2 near real-time (NRT) and off-line (OL) ESA processors that have been
used to derive level 2 geophysical products from the calibrated and
geolocated level&amp;nbsp;1b spectra. The design of the code and the analysis
methodology have been driven by the requirements for NRT processing. This
paper reviews the performance of the optimised retrieval strategy that has
been implemented to achieve these requirements and provides estimated error
budgets for the target products: pressure/temperature, O&lt;sub&gt;3&lt;/sub&gt;, H&lt;sub&gt;2&lt;/sub&gt;O,
CH&lt;sub&gt;4&lt;/sub&gt;, HNO&lt;sub&gt;3&lt;/sub&gt;, N&lt;sub&gt;2&lt;/sub&gt;O and NO&lt;sub&gt;2&lt;/sub&gt;, in the altitude measurement
range from 6 to 68 km.

&lt;br&gt;&lt;br&gt;
From application to real MIPAS data, it was found that no change was needed
in the developed code although an external algorithm was introduced to
identify clouds with high opacity and to exclude affected spectra from the
analysis. In addition, a number of updates were made to the set-up
parameters and to auxiliary data. In particular, a new version of the MIPAS
dedicated spectroscopic database was used and, in the OL analysis, the
retrieval range was extended to reduce errors due to uncertainties in
extrapolation of the profile outside the retrieval range and more stringent
convergence criteria were implemented.

&lt;br&gt;&lt;br&gt;
A statistical analysis on the &amp;chi;&lt;sup&gt;2&lt;/sup&gt; values obtained in one year of
measurements shows good agreement with the a priori estimate of the forward
model errors. On the basis of the first two years of MIPAS measurements the
estimates of the forward model and instrument errors are in general found to
be conservative with excellent performance demonstrated for frequency
calibration. It is noted that the total retrieval error is limited by
forward model errors which make useless a further reduction of random
errors. However, such a reduction is within the capabilities of MIPAS
measurements, which contain many more spectral signatures of the target
species than what currently used. Further work is needed to reduce the
amplitude of the forward model errors, so that the random error and the
total error budget can be reduced accordingly.

&lt;br&gt;&lt;br&gt;
The importance of the Averaging kernels for a full characterisation of the
target products is underlined and the equations are provided for their
practical applications.</abstract>
	<references>
	</references>
</article>

