<?xml version="1.0" encoding="utf-8" standalone="no"?>
<!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>5</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/acpd-5-7929-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/7929/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/7929/2005/acpd-5-7929-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/7929/2005/acpd-5-7929-2005.pdf</fulltext_pdf>
	<start_page>7929</start_page>
	<end_page>7964</end_page>
	<publication_date>2005-09-02</publication_date>
	<article_title content_type="html">Intercomparison exercise between different radiative transfer models used for the interpretation of ground-based zenith-sky and multi-axis DOAS observations</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>F. Hendrick</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>M. Van Roozendael</name>
		</author>
		<author numeration="3" affiliations="2,7">
			<name>A. Kylling</name>
		</author>
		<author numeration="4" affiliations="3">
			<name>A. Petritoli</name>
		</author>
		<author numeration="5" affiliations="4">
			<name>A. Rozanov</name>
		</author>
		<author numeration="6" affiliations="5">
			<name>S. Sanghavi</name>
		</author>
		<author numeration="7" affiliations="6,8">
			<name>R. Schofield</name>
		</author>
		<author numeration="8" affiliations="5">
			<name>C. von Friedeburg</name>
		</author>
		<author numeration="9" affiliations="5">
			<name>T. Wagner</name>
		</author>
		<author numeration="10" affiliations="4">
			<name>F. Wittrock</name>
		</author>
		<author numeration="11" affiliations="1">
			<name>D. Fonteyn</name>
		</author>
		<author numeration="12" affiliations="1">
			<name>M. De Mazière</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institut d’Aéronomie Spatiale de Belgique, Brussels, Belgium</affiliation>
		<affiliation numeration="2" content_type="html">Norwegian Institute for Air Research, Kjeller, Norway</affiliation>
		<affiliation numeration="3" content_type="html">Institute of Atmospheric Science and Climate, Bologna, Italy</affiliation>
		<affiliation numeration="4" content_type="html">Institute of Environmental Physics, University of Bremen, Bremen, Germany</affiliation>
		<affiliation numeration="5" content_type="html">Institute of Environmental Physics, University of Heidelberg, Heidelberg, Germany</affiliation>
		<affiliation numeration="6" content_type="html">National Institute of Water and Atmospheric Research, Omakau, Central Otago, New Zealand</affiliation>
		<affiliation numeration="7" content_type="html">now at: St. Olavs University Hospital, Trondheim, Norway</affiliation>
		<affiliation numeration="8" content_type="html">now at: NOAA Aeronomy Laboratory, Boulder, Colorado, USA</affiliation>
	</affiliations>
	<abstract content_type="html">We present the results of an intercomparison exercise between six different
radiative transfer (RT) models carried out in the framework of QUILT, an EU
funded project based on the exploitation of the Network for the Detection of
Stratospheric Change (NDSC). RT modeling is an important step in the
interpretation of Differential Optical Absorption Spectroscopy (DOAS)
observations. It allows the conversion of the slant column densities (SCDs)
into vertical column densities (VCDs) using calculated air mass factors
(AMFs). The originality of our study resides in comparing SCD simulations in
multi-axis (MAX) geometry (trace gases: NO&lt;sub&gt;2&lt;/sub&gt; and HCHO) and in taking
into account the photochemical enhancement for calculating SCDs of rapidly
photolysing species (BrO, NO&lt;sub&gt;2&lt;/sub&gt;, and OClO) in zenith-sky geometry.
Concerning the MAX simulations, good agreement is observed between the
different models with the calculated NO&lt;sub&gt;2&lt;/sub&gt; and HCHO SCDs differing by no
more than 5% in the elevation and solar zenith angles (SZA) ranges
investigated (5&amp;deg;&amp;ndash;20&amp;deg; and 35&amp;deg;&amp;ndash;85&amp;deg;, respectively). The impacts
of aerosol scattering, ground albedo, and relative azimuth on MAX
simulations have also been tested. Large discrepancies appear for the
aerosol effect, suggesting differences between models in the treatment of
the aerosol scattering. A better agreement is obtained in the case of the
ground albedo and relative azimuth effects. In zenith-sky geometry, the
different models agree generally well, especially below 90&amp;deg; SZA. At
higher SZA, larger discrepancies are observed with relative difference
values between 2% and 14% in some cases. All the initialization data
and results have been made publicly available through the QUILT project web
site (http://nadir.nilu.no/quilt/), enabling the testing of other RT codes
designed for the calculation of SCDs/AMFs.</abstract>
	<references>
	</references>
</article>

