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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>6</volume_number>
		<issue_number>5</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acpd-6-10153-2006</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/6/10153/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/6/10153/2006/acpd-6-10153-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/6/10153/2006/acpd-6-10153-2006.pdf</fulltext_pdf>
	<start_page>10153</start_page>
	<end_page>10182</end_page>
	<publication_date>2006-10-12</publication_date>
	<article_title content_type="html">On the variability of the Ring effect in the near ultraviolet: understanding the role of aerosols and multiple scattering</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>A. O. Langford</name>
		</author>
		<author numeration="2" affiliations="1,3,4">
			<name>R. Schofield</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>J. S. Daniel</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>R. W. Portmann</name>
		</author>
		<author numeration="5" affiliations="1,3">
			<name>M. L. Melamed</name>
		</author>
		<author numeration="6" affiliations="1,3">
			<name>H. L. Miller</name>
		</author>
		<author numeration="7" affiliations="2">
			<name>E. G. Dutton</name>
		</author>
		<author numeration="8" affiliations="1">
			<name>S. Solomon</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">NOAA Earth System Research Laboratory/Chemical Sciences Division, Boulder, Colorado, USA</affiliation>
		<affiliation numeration="2" content_type="html">NOAA Earth System Research Laboratory/Global Monitoring Division, Boulder, Colorado, USA</affiliation>
		<affiliation numeration="3" content_type="html">CIRES, University of Colorado, Boulder, Colorado, USA</affiliation>
		<affiliation numeration="4" content_type="html">now at: Alfred-Wegener-Institute for Polar and Marine Research, Research Department Potsdam, Potsdam, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">The &quot;filling-in&apos;&apos; (FI) of Fraunhofer lines, often referred to as the Ring
effect, was examined using measurements of near ultraviolet sunlight
scattered from the zenith sky above Boulder, Colorado during July and August
2005. The FI of the 344.1 nm Fe I line was directly determined by comparing
direct sun and cloud-free zenith sky spectra recorded on the same day. The
results, obtained over solar zenith angles (SZA) from 20 to 70&amp;deg;, are
compared to the predictions of a simple Rotational Raman Scattering (RRS)
spectral model. The measured FI was found to be up to 70% greater than
that predicted by first-order molecular scattering with a much stronger SZA
dependence. Simultaneously measured aerosol optical depths and Monte Carlo
calculations show that the combination of aerosol scattering and
second-order molecular scattering can account for these differences, and
potentially explain the contradictory SZA dependences in previously
published measurements of FI. These two scattering processes also introduce
a wavelength dependence to FI that complicates the fitting of diffuse
sunlight observations in differential optical absorption spectroscopy
(DOAS). A simple correction to improve DOAS retrievals by removing this
wavelength dependence is described.</abstract>
	<references>
	</references>
</article>

