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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>10</volume_number>
		<issue_number>3</issue_number>
		<publication_year>2010</publication_year>
	</journal>
	<doi>10.5194/acpd-10-6755-2010</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/10/6755/2010/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/10/6755/2010/acpd-10-6755-2010.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/10/6755/2010/acpd-10-6755-2010.pdf</fulltext_pdf>
	<start_page>6755</start_page>
	<end_page>6796</end_page>
	<publication_date>2010-03-11</publication_date>
	<article_title content_type="html">GOMOS data characterization and error estimation</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J. Tamminen</name>
			<email>johanna.tamminen@fmi.fi</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>E. KyrÃ¶lÃ¤</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>V. F. Sofieva</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>M. Laine</name>
		</author>
		<author numeration="5" affiliations="2">
			<name>J.-L. Bertaux</name>
		</author>
		<author numeration="6" affiliations="2">
			<name>A. Hauchecorne</name>
		</author>
		<author numeration="7" affiliations="2">
			<name>F. Dalaudier</name>
		</author>
		<author numeration="8" affiliations="3">
			<name>D. Fussen</name>
		</author>
		<author numeration="9" affiliations="3">
			<name>F. Vanhellemont</name>
		</author>
		<author numeration="10" affiliations="4">
			<name>O. Fanton-d&apos;Andon</name>
		</author>
		<author numeration="11" affiliations="4">
			<name>G. Barrot</name>
		</author>
		<author numeration="12" affiliations="4">
			<name>A. Mangin</name>
		</author>
		<author numeration="13" affiliations="4">
			<name>M. Guirlet</name>
		</author>
		<author numeration="14" affiliations="4">
			<name>L. Blanot</name>
		</author>
		<author numeration="15" affiliations="5">
			<name>T. Fehr</name>
		</author>
		<author numeration="16" affiliations="5">
			<name>L. Saavedra de Miguel</name>
		</author>
		<author numeration="17" affiliations="6">
			<name>R. Fraisse</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Finnish Meteorological Institute, Earth Observation, Helsinki, Finland</affiliation>
		<affiliation numeration="2" content_type="html">Service d&apos;Aeronomie, Paris, France</affiliation>
		<affiliation numeration="3" content_type="html">BIRA-IASB, Brussels, Belgium</affiliation>
		<affiliation numeration="4" content_type="html">ACRI ST, Sophia Antipolis, France</affiliation>
		<affiliation numeration="5" content_type="html">ESA-ESRIN, Italy</affiliation>
		<affiliation numeration="6" content_type="html">EADS-Astrium, Toulouse, France</affiliation>
	</affiliations>
	<abstract content_type="html">The Global Ozone Monitoring by Occultation of Stars
(GOMOS) instrument uses stellar occultation technique for monitoring
ozone and other trace gases in the stratosphere and mesosphere. The
self-calibrating measurement principle of GOMOS together with
a relatively simple data retrieval where only minimal use of a priori
data is required, provides excellent possibilities for long term
monitoring of atmospheric composition.
&lt;br&gt;&lt;br&gt;
GOMOS uses about 180 brightest stars as the light source. Depending on
the individual spectral characteristics of the stars, the
signal-to-noise
ratio of GOMOS is changing from star to star, resulting also
varying accuracy to the retrieved profiles. We present the overview
of the GOMOS data characterization and error estimation,
including modeling errors, for ozone,
NO&lt;sub&gt;2&lt;/sub&gt;, NO&lt;sub&gt;3&lt;/sub&gt;
and aerosol
profiles. The retrieval error (precision) of the night time measurements in
the stratosphere is typically 0.5â€“4% for ozone, about 10â€“20% for NO&lt;sub&gt;2&lt;/sub&gt;,
20&amp;ndash;40% for NO&lt;sub&gt;3&lt;/sub&gt; and 2â€“50% for aerosols. Mesospheric O&lt;sub&gt;3&lt;/sub&gt;,
up to 100 km,  can
be measured with 2â€“10% precision.
The main sources of the modeling error are the
incompletely corrected
atmospheric turbulence causing scintillation, inaccurate aerosol
modeling, uncertainties in cross sections of the trace gases and in
the atmospheric temperature. The sampling resolution of GOMOS varies
depending on the measurement geometry. In the data inversion a Tikhonov-type
regularization with pre-defined target resolution requirement is applied
leading to 2â€“3 km resolution for ozone and 4 km resolution for other
trace gases.</abstract>
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</article>

