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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>8</volume_number>
		<issue_number>3</issue_number>
		<publication_year>2008</publication_year>
	</journal>
	<doi>10.5194/acpd-8-10301-2008</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/8/10301/2008/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/8/10301/2008/acpd-8-10301-2008.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/8/10301/2008/acpd-8-10301-2008.pdf</fulltext_pdf>
	<start_page>10301</start_page>
	<end_page>10352</end_page>
	<publication_date>2008-06-02</publication_date>
	<article_title content_type="html">Photolysis frequency measurement techniques: results of a comparison within the ACCENT project</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>B. Bohn</name>
			<email>b.bohn@fz-juelich.de</email>
		</author>
		<author numeration="2" affiliations="2">
			<name>G. K. Corlett</name>
		</author>
		<author numeration="3" affiliations="3,11">
			<name>M. Gillmann</name>
		</author>
		<author numeration="4" affiliations="3">
			<name>S. Sanghavi</name>
		</author>
		<author numeration="5" affiliations="4">
			<name>G. Stange</name>
		</author>
		<author numeration="6" affiliations="4">
			<name>E. Tensing</name>
		</author>
		<author numeration="7" affiliations="5,12">
			<name>M. Vrekoussis</name>
		</author>
		<author numeration="8" affiliations="6,13">
			<name>W. J. Bloss</name>
		</author>
		<author numeration="9" affiliations="7">
			<name>L. J. Clapp</name>
		</author>
		<author numeration="10" affiliations="8,14">
			<name>M. Kortner</name>
		</author>
		<author numeration="11" affiliations="1">
			<name>H.-P. Dorn</name>
		</author>
		<author numeration="12" affiliations="2">
			<name>P. S. Monks</name>
		</author>
		<author numeration="13" affiliations="3">
			<name>U. Platt</name>
		</author>
		<author numeration="14" affiliations="4">
			<name>C. Plass-Dülmer</name>
		</author>
		<author numeration="15" affiliations="5">
			<name>N. Mihalopoulos</name>
		</author>
		<author numeration="16" affiliations="6">
			<name>D. E. Heard</name>
		</author>
		<author numeration="17" affiliations="7,15">
			<name>K. C. Clemitshaw</name>
		</author>
		<author numeration="18" affiliations="8">
			<name>F. X. Meixner</name>
		</author>
		<author numeration="19" affiliations="9">
			<name>A. S. H. Prevot</name>
		</author>
		<author numeration="20" affiliations="10">
			<name>R. Schmitt</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institut für Chemie und Dynamik der Geosphäre 2:  Troposphäre, Forschungszentrum Jülich, 52425 Jülich,  Germany</affiliation>
		<affiliation numeration="2" content_type="html">Department of Chemistry, University of Leicester,  Leicester LE1 7RH, UK</affiliation>
		<affiliation numeration="3" content_type="html">Institut für Umweltphysik, Universität  Heidelberg, 69120 Heidelberg, Germany</affiliation>
		<affiliation numeration="4" content_type="html">Deutscher Wetterdienst, Meteorologisches Observatorium  Hohenpeissenberg, 82383 Hohenpeissenberg, Germany</affiliation>
		<affiliation numeration="5" content_type="html">Environmental Chemistry Laboratory, University of Crete,  71003 Voutes, Heraklion, Greece</affiliation>
		<affiliation numeration="6" content_type="html">School of Chemistry, University of Leeds, Leeds LS2 9JT,  UK</affiliation>
		<affiliation numeration="7" content_type="html">Department of Environmental Science and Technology,  Imperial College London, Silwood Park Campus, Ascot SL5 7PY,  UK</affiliation>
		<affiliation numeration="8" content_type="html">Biogeochemistry Department, Max Planck Institute for  Chemistry, 55128 Mainz, Germany</affiliation>
		<affiliation numeration="9" content_type="html">Laboratory of Atmospheric Chemistry, Paul Scherrer  Institute, 5232 Villigen, Switzerland</affiliation>
		<affiliation numeration="10" content_type="html">Meteorologie Consult GmbH (Metcon GmbH), 61462 Königstein,  Germany</affiliation>
		<affiliation numeration="11" content_type="html">now at: SIG Plasmax GmbH, 22145 Hamburg, Germany</affiliation>
		<affiliation numeration="12" content_type="html">now at: Institut für Umweltphysik, University of  Bremen, 28359 Bremen, Germany</affiliation>
		<affiliation numeration="13" content_type="html">now at: School of Geography, Earth &amp; Environmental  Sciences, University of Birmingham, Birmingham B15 2TT, UK</affiliation>
		<affiliation numeration="14" content_type="html">now at: Müller-BBM GmbH, 63589 Linsengericht,  Germany</affiliation>
		<affiliation numeration="15" content_type="html">now at: Department of Earth Sciences, Royal  Holloway, University of London, Egham TW20 0EX, UK</affiliation>
	</affiliations>
	<abstract content_type="html">An intercomparison of different
radiometric techniques measuring atmospheric photolysis
frequencies &lt;I&gt;j&lt;/I&gt;(NO&lt;sub&gt;2&lt;/sub&gt;), &lt;I&gt;j&lt;/I&gt;(HCHO) and &lt;I&gt;j&lt;/I&gt;(O&lt;sup&gt;1&lt;/sup&gt;D) was carried out
in a two-week field campaign in June 2005 at Jülich, Germany.
Three double-monochromator based spectroradiometers (DM-SR), three
single-monochromator based spectroradiometers with diode-array
detectors (SM-SR) and seventeen filter radiometers (FR) (ten
&lt;I&gt;j&lt;/I&gt;(NO&lt;sub&gt;2&lt;/sub&gt;)-FR, seven &lt;I&gt;j&lt;/I&gt;(O&lt;sup&gt;1&lt;/sup&gt;D)-FR) took part in this
comparison. For &lt;I&gt;j&lt;/I&gt;(NO&lt;sub&gt;2&lt;/sub&gt;), all spectroradiometer results agreed
within &amp;plusmn;3%. For &lt;I&gt;j&lt;/I&gt;(HCHO), agreement was slightly poorer
between &amp;minus;8% and +4% of the DM-SR reference result. For the
SM-SR deviations were explained by poorer spectral resolutions and
lower accuracies caused by decreased sensitivities of the
photodiode arrays in a wavelength range below 350 nm. For
&lt;I&gt;j&lt;/I&gt;(O&lt;sup&gt;1&lt;/sup&gt;D), the results were more complex within +8% and &amp;minus;4%
with increasing deviations towards larger solar zenith angles for
the SM-SR. The direction and the magnitude of the deviations were
dependent on the technique of background determination. All
&lt;I&gt;j&lt;/I&gt;(NO&lt;sub&gt;2&lt;/sub&gt;)-FR showed good linearity with single calibration
factors being sufficient to convert from output voltages to
&lt;I&gt;j&lt;/I&gt;(NO&lt;sub&gt;2&lt;/sub&gt;). Measurements were feasible until sunset and
comparison with previous calibrations showed good long-term
stability. For the &lt;I&gt;j&lt;/I&gt;(O&lt;sup&gt;1&lt;/sup&gt;D)-FR, conversion from output voltages
to &lt;I&gt;j&lt;/I&gt;(O&lt;sup&gt;1&lt;/sup&gt;D) needed calibration factors and correction functions
considering the influences of total ozone column and altitude of
the sun. All instruments showed good linearity at photolysis
frequencies exceeding about 10% of maximum values. At larger
solar zenith angles, the agreement was non-uniform with deviations
explainable by insufficient correction functions. Comparison with
previous calibrations for some &lt;I&gt;j&lt;/I&gt;(O&lt;sup&gt;1&lt;/sup&gt;D)-FR indicated drifts of
calibration factors.</abstract>
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</article>

