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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>1</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/acpd-5-17-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/17/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/17/2005/acpd-5-17-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/17/2005/acpd-5-17-2005.pdf</fulltext_pdf>
	<start_page>17</start_page>
	<end_page>66</end_page>
	<publication_date>2005-01-10</publication_date>
	<article_title content_type="html">Solar occultation with SCIAMACHY: algorithm description and first validation</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J. Meyer</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>A. Bracher</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>A. Rozanov</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>A. C. Schlesier</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>H. Bovensmann</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>J. P. Burrows</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institute of Environmental Physics, University of Bremen, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">This presentation concentrates on solar occultation measurements with the
spaceborne spectrometer SCIAMACHY in the UV-Vis wavelength range. Solar
occultation measurements provide unique information about the vertical
distribution of atmospheric constituents. For retrieval of vertical trace gas
concentration profiles, an algorithm has been developed based on the optimal
estimation method. The forward model is capable to simulate the extinction
signals of different species as they occur in atmospheric transmission
spectra obtained from occultation measurements. Furthermore, correction
algorithms have been implemented to address shortcomings of the tangent
height pre-processing and inhomogeneities of measured solar spectra. First
results of O&lt;sub&gt;3&lt;/sub&gt; and NO&lt;sub&gt;2&lt;/sub&gt; vertical profile retrievals have been validated
with data from ozone sondes and satellite based occultation instruments. The
validation shows very promising results for SCIAMACHY O&lt;sub&gt;3&lt;/sub&gt; and NO&lt;sub&gt;2&lt;/sub&gt; values
between 15 to 35 km with errors in the order of 10% and 15%,
respectively.</abstract>
	<references>
	</references>
</article>

