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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>3</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acpd-6-3513-2006</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/6/3513/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/6/3513/2006/acpd-6-3513-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/6/3513/2006/acpd-6-3513-2006.pdf</fulltext_pdf>
	<start_page>3513</start_page>
	<end_page>3570</end_page>
	<publication_date>2006-05-05</publication_date>
	<article_title content_type="html">A modified band approach for the accurate calculation of on-line photolysis rates in stratospheric-tropospheric Chemical Transport Models</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J. E. Williams</name>
		</author>
		<author numeration="2" affiliations="2">
			<name>J. Landgraf</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>A. Bregman</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>H. Walter</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Royal Netherlands Meteorological Institute, De Bilt, The Netherlands</affiliation>
		<affiliation numeration="2" content_type="html">SRON National Institute for Space Research, Utrecht, The Netherlands</affiliation>
	</affiliations>
	<abstract content_type="html">Here we present an efficient and accurate method for the online calculation
of photolysis rates relevant to both the stratosphere and troposphere for
use in global Chemistry Transport Models. The method is a modified version
of the band model introduced by Landgraf and Crutzen (1998) which has been
updated to improve the performance of the approach for solar zenith angles
&amp;gt;75&amp;deg; without the use of any implicit parameterisations. For this
purpose, additional sets of band parameters have been defined for instances
where the incident angle of the light beam is between 75&amp;ndash;93&amp;deg;, in
conjunction with a scaling component for the far UV region of the spectrum
(&amp;lambda;=176.6&amp;ndash;202.0 nm). For incident angles between 85&amp;ndash;93&amp;deg; we
introduce a modification for pseudo-sphericity that improves the accuracy of
the 2-stream approximation. We show that this modified version of PIFM is
accurate for angles &amp;lt;93&amp;deg; by comparing the resulting height resolved
actinic fluxes with a recently developed full spherical reference model. We
also show that the modified band method is more accurate than the original,
with errors generally being &amp;plusmn;10% throughout the atmospheric column
for a diverse range of chemical species. Moreover, we perform certain
sensitivity studies that indicate it is robust and performs well over a wide
range of conditions relevant to the atmosphere.</abstract>
	<references>
	</references>
</article>

