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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>5</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acpd-6-9765-2006</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/6/9765/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/6/9765/2006/acpd-6-9765-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/6/9765/2006/acpd-6-9765-2006.pdf</fulltext_pdf>
	<start_page>9765</start_page>
	<end_page>9821</end_page>
	<publication_date>2006-10-05</publication_date>
	<article_title content_type="html">Validation of MIPAS ClONO&lt;sub&gt;2&lt;/sub&gt; measurements</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>M. Höpfner</name>
		</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>S. Kellmann</name>
		</author>
		<author numeration="8" affiliations="1">
			<name>M. Kiefer</name>
		</author>
		<author numeration="9" affiliations="1">
			<name>A. Linden</name>
		</author>
		<author numeration="10" affiliations="1">
			<name>M. Milz</name>
		</author>
		<author numeration="11" affiliations="1">
			<name>T. Steck</name>
		</author>
		<author numeration="12" affiliations="1">
			<name>G. P. Stiller</name>
		</author>
		<author numeration="13" affiliations="3">
			<name>P. Bernath</name>
		</author>
		<author numeration="14" affiliations="1">
			<name>C. E. Blom</name>
		</author>
		<author numeration="15" affiliations="1">
			<name>Th. Blumenstock</name>
		</author>
		<author numeration="16" affiliations="3">
			<name>C. Boone</name>
		</author>
		<author numeration="17" affiliations="4">
			<name>K. Chance</name>
		</author>
		<author numeration="18" affiliations="5">
			<name>M. T. Coffey</name>
		</author>
		<author numeration="19" affiliations="1">
			<name>F. Friedl-Vallon</name>
		</author>
		<author numeration="20" affiliations="6">
			<name>D. Griffith</name>
		</author>
		<author numeration="21" affiliations="5">
			<name>J. W. Hannigan</name>
		</author>
		<author numeration="22" affiliations="1">
			<name>F. Hase</name>
		</author>
		<author numeration="23" affiliations="6">
			<name>N. Jones</name>
		</author>
		<author numeration="24" affiliations="7">
			<name>K. W. Jucks</name>
		</author>
		<author numeration="25" affiliations="1">
			<name>C. Keim</name>
		</author>
		<author numeration="26" affiliations="1">
			<name>A. Kleinert</name>
		</author>
		<author numeration="27" affiliations="1">
			<name>W. Kouker</name>
		</author>
		<author numeration="28" affiliations="1">
			<name>G. Y. Liu</name>
		</author>
		<author numeration="29" affiliations="8">
			<name>E. Mahieu</name>
		</author>
		<author numeration="30" affiliations="9">
			<name>J. Mellqvist</name>
		</author>
		<author numeration="31" affiliations="1">
			<name>S. Mikuteit</name>
		</author>
		<author numeration="32" affiliations="10">
			<name>J. Notholt</name>
		</author>
		<author numeration="33" affiliations="1">
			<name>H. Oelhaf</name>
		</author>
		<author numeration="34" affiliations="1">
			<name>C. Piesch</name>
		</author>
		<author numeration="35" affiliations="1">
			<name>T. Reddmann</name>
		</author>
		<author numeration="36" affiliations="1">
			<name>R. Ruhnke</name>
		</author>
		<author numeration="37" affiliations="1">
			<name>M. Schneider</name>
		</author>
		<author numeration="38" affiliations="9">
			<name>A. Strandberg</name>
		</author>
		<author numeration="39" affiliations="11">
			<name>G. Toon</name>
		</author>
		<author numeration="40" affiliations="3">
			<name>K. A. Walker</name>
		</author>
		<author numeration="41" affiliations="10">
			<name>T. Warneke</name>
		</author>
		<author numeration="42" affiliations="1">
			<name>G. Wetzel</name>
		</author>
		<author numeration="43" affiliations="12">
			<name>S. Wood</name>
		</author>
		<author numeration="44" affiliations="8">
			<name>R. Zander</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 Astrof&amp;#237;sica de Andaluc&amp;#237;a, Granada, Spain</affiliation>
		<affiliation numeration="3" content_type="html">Department of Chemistry, University of Waterloo, Ontario, Canada</affiliation>
		<affiliation numeration="4" content_type="html">Harvard-Smithsonian Center for Astrophysics, Atomic and Molecular Physics Division, Cambridge, MA, USA</affiliation>
		<affiliation numeration="5" content_type="html">Atmospheric Chemistry Division, National Center for Atmospheric Research, Boulder, CO, USA</affiliation>
		<affiliation numeration="6" content_type="html">Department of Chemistry, University of Wollongong, Australia</affiliation>
		<affiliation numeration="7" content_type="html">Harvard-Smithsonian Center for Astrophysics, Optical and Infrared Astronomy Division, Cambridge, MA, USA</affiliation>
		<affiliation numeration="8" content_type="html">Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium</affiliation>
		<affiliation numeration="9" content_type="html">Department of Radio and Space Science, Chalmers University of Technology, G¨oteborg, Sweden</affiliation>
		<affiliation numeration="10" content_type="html">Institut für Umweltphysik, Universität Bremen, Germany</affiliation>
		<affiliation numeration="11" content_type="html">Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA</affiliation>
		<affiliation numeration="12" content_type="html">National Institute of Water and Atmospheric Research, Lauder, New-Zealand</affiliation>
	</affiliations>
	<abstract content_type="html">Altitude profiles of ClONO&lt;sub&gt;2&lt;/sub&gt; retrieved with the IMK (Institut f&amp;#252;r
Meteorologie und Klimaforschung) science-oriented data processor from
MIPAS/Envisat (Michelson Interferometer for Passive Atmospheric Sounding on
Envisat) mid-infrared limb emission measurements between July 2002 and March
2004 have been validated by comparison with balloon-borne (Mark&amp;nbsp;IV, FIRS2,
MIPAS-B), airborne (MIPAS-STR), ground-based (Spitsbergen, Thule, Kiruna,
Harestua, Jungfraujoch, Iza&amp;#241;a, Wollongong, Lauder), and spaceborne
(ACE-FTS) observations. With few exceptions we found very good agreement
between these instruments and MIPAS with no evidence for any bias in most
cases and altitude regions. For balloon-borne measurements typical absolute
mean differences are below 0.05 ppbv over the whole altitude range from 10 to
39 km. In case of ACE-FTS observations mean differences are below 0.03 ppbv
for observations below 26 km. Above this altitude the comparison with ACE-FTS
is affected by the photochemically induced diurnal variation of ClONO&lt;sub&gt;2&lt;/sub&gt;.
Correction for this by use of a chemical transport model led to an
overcompensation of the photochemical effect by up to 0.1 ppbv at altitudes
of 30&amp;ndash;35 km in case of MIPAS-ACE-FTS comparisons while for the balloon-borne
observations no such inconsistency has been detected. The comparison of MIPAS
derived total column amounts with ground-based observations revealed no
significant bias in the MIPAS data. Mean differences between MIPAS and FTIR
column abundances are 0.11&amp;plusmn;0.12&amp;times;10&lt;sup&gt;14&lt;/sup&gt; cm&lt;sup&gt;&amp;minus;2&lt;/sup&gt; (1.0&amp;plusmn;1.1%)
and &amp;minus;0.09&amp;plusmn;0.19&amp;times;10&lt;sup&gt;14&lt;/sup&gt; cm&lt;sup&gt;&amp;minus;2&lt;/sup&gt; (&amp;minus;0.8&amp;plusmn;1.7%), depending on
the coincidence criterion applied. &amp;chi;&lt;sup&gt;2&lt;/sup&gt; tests have been performed to
assess the combined precision estimates of MIPAS and the related instruments.
When no exact coincidences were available as in case of MIPAS &amp;ndash; FTIR or MIPAS
&amp;ndash; ACE-FTS comparisons it has been necessary to take into consideration a
coincidence error term to account for &amp;chi;&lt;sup&gt;2&lt;/sup&gt; deviations. From the resulting
&amp;chi;&lt;sup&gt;2&lt;/sup&gt; profiles there is no evidence for a systematic over/underestimation
of the MIPAS random error analysis.</abstract>
	<references>
	</references>
</article>

