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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>8</volume_number>
		<issue_number>2</issue_number>
		<publication_year>2008</publication_year>
	</journal>
	<doi>10.5194/acpd-8-5183-2008</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/8/5183/2008/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/8/5183/2008/acpd-8-5183-2008.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/8/5183/2008/acpd-8-5183-2008.pdf</fulltext_pdf>
	<start_page>5183</start_page>
	<end_page>5233</end_page>
	<publication_date>2008-03-11</publication_date>
	<article_title content_type="html">Error analysis for CO and CH&lt;sub&gt;4&lt;/sub&gt; total column retrievals from  SCIAMACHY 2.3 μm spectra</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>A. M. S. Gloudemans</name>
			<email>a.gloudemans@sron.nl</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>H. Schrijver</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>O. P. Hasekamp</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>I. Aben</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">SRON Netherlands Institute for Space Research, Utrecht, The Netherlands</affiliation>
	</affiliations>
	<abstract content_type="html">A detailed sensitivity analysis of the Iterative Maximum Likelihood
Method (IMLM) algorithm and its application
to the SCIAMACHY 2.3 μm spectra is presented.
The sensitivity analysis includes a detailed assessment of the impact of
aerosols in the 2.3 μm range.
Results show that near strong aerosol sources mineral
dust and biomass aerosols can have an effect of ~7&amp;ndash;10%
on the CH&lt;sub&gt;4&lt;/sub&gt; total columns retrieved from this wavelength range. Similar
but somewhat larger effects are found for CO, but due to the
larger variability of CO
these errors are less important. Away from strong sources much
smaller effects of a few percent are found.
Spectroscopic uncertainties are mostly negligible except for
uncertainties in the CH&lt;sub&gt;4&lt;/sub&gt; intrinsic line intensities, which can
be important.
Application of the IMLM algorithm
to the SCIAMACHY 2.3 μm spectra shows that the
quality of the retrieved CO and CH&lt;sub&gt;4&lt;/sub&gt; total columns is good, except
for a bias for large instrument-noise errors which is partly due to
remaining calibration issues.
Polarization sensitivity of the SCIAMACHY instrument has a negligible effect
on the retrieved CO and CH&lt;sub&gt;4&lt;/sub&gt; total columns.
The H&lt;sub&gt;2&lt;/sub&gt;O total
columns, which have to be retrieved simultaneously with CO and CH&lt;sub&gt;4&lt;/sub&gt;
due to overlapping absorption lines, agree
well with H&lt;sub&gt;2&lt;/sub&gt;O total columns from ECMWF data.
This ensures that the fit to the
H&lt;sub&gt;2&lt;/sub&gt;O absorptions is of sufficient quality not to hamper
the retrieved CO and CH&lt;sub&gt;4&lt;/sub&gt; total columns from SCIAMACHY spectra.</abstract>
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</article>

