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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>4</issue_number>
		<publication_year>2010</publication_year>
	</journal>
	<doi>10.5194/acpd-10-11109-2010</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/10/11109/2010/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/10/11109/2010/acpd-10-11109-2010.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/10/11109/2010/acpd-10-11109-2010.pdf</fulltext_pdf>
	<start_page>11109</start_page>
	<end_page>11138</end_page>
	<publication_date>2010-04-26</publication_date>
	<article_title content_type="html">Optical extinction by upper tropospheric/stratospheric aerosols and clouds: GOMOS observations for the period 2002–2008</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>F. Vanhellemont</name>
			<email>filip.vanhellemont@aeronomie.be</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>D. Fussen</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>N. Mateshvili</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>C. Tétard</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>C. Bingen</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>E. Dekemper</name>
		</author>
		<author numeration="7" affiliations="1">
			<name>N. Loodts</name>
		</author>
		<author numeration="8" affiliations="2">
			<name>E. Kyrölä</name>
		</author>
		<author numeration="9" affiliations="2">
			<name>V. Sofieva</name>
		</author>
		<author numeration="10" affiliations="2">
			<name>J. Tamminen</name>
		</author>
		<author numeration="11" affiliations="3">
			<name>A. Hauchecorne</name>
		</author>
		<author numeration="12" affiliations="3">
			<name>J.-L. Bertaux</name>
		</author>
		<author numeration="13" affiliations="3">
			<name>F. Dalaudier</name>
		</author>
		<author numeration="14" affiliations="3,4">
			<name>L. Blanot</name>
		</author>
		<author numeration="15" affiliations="4">
			<name>O. Fanton d&apos;Andon</name>
		</author>
		<author numeration="16" affiliations="4">
			<name>G. Barrot</name>
		</author>
		<author numeration="17" affiliations="4">
			<name>M. Guirlet</name>
		</author>
		<author numeration="18" affiliations="5">
			<name>T. Fehr</name>
		</author>
		<author numeration="19" affiliations="5">
			<name>L. Saavedra</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Belgian Institute for Space Aeronomy, Brussels, Belgium</affiliation>
		<affiliation numeration="2" content_type="html">Finnish Meteorological Institute, Helsinki, Finland</affiliation>
		<affiliation numeration="3" content_type="html">Service d&apos;Aéronomie du CNRS, Verrieres-le-Buisson, France</affiliation>
		<affiliation numeration="4" content_type="html">ACRI-ST, Sophia-Antipolis, France</affiliation>
		<affiliation numeration="5" content_type="html">ESA-ESRIN, Frascati, Italy</affiliation>
	</affiliations>
	<abstract content_type="html">Although the retrieval of aerosol extinction coefficients from satellite
remote measurements is notoriously difficult (in comparison with gaseous
species) due to the lack of typical spectral signatures, important
information can be obtained. In this paper we present an overview of the
current operational nighttime UV/Vis aerosol extinction profile results for
the GOMOS star occultation instrument, spanning the period from August 2002
to May 2008. Some problems still remain, such as the ones associated with
incomplete scintillation correction and the aerosol spectral law
implementation, but good quality extinction values can be expected at a
wavelength of 500 nm. Typical phenomena associated with atmospheric
particulate matter in the Upper Troposphere/Lower Stratosphere (UTLS) are
easily identified: Polar Stratospheric Clouds, tropical subvisual cirrus
clouds, background stratospheric aerosols, and post-eruption volcanic
aerosols (with their subsequent dispersion around the globe). In this
overview paper we will give a summary of the current results.</abstract>
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</article>

