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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>4</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2004</publication_year>
	</journal>
	<doi>10.5194/acpd-4-4191-2004</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/4/4191/2004/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/4/4191/2004/acpd-4-4191-2004.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/4/4191/2004/acpd-4-4191-2004.pdf</fulltext_pdf>
	<start_page>4191</start_page>
	<end_page>4225</end_page>
	<publication_date>2004-08-04</publication_date>
	<article_title content_type="html">Actinic flux and O&lt;sup&gt;1&lt;/sup&gt;D photolysis frequencies retrieved from spectral measurements of irradiance at Thessaloniki, Greece</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>S. Kazadzis</name>
			<email>skaza@skiathos.physics.auth.gr</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>C. Topaloglou</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>A. F. Bais</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>M. Blumthaler</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>D. Balis</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>A. Kazantzidis</name>
		</author>
		<author numeration="7" affiliations="2">
			<name>B. Schallhart</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Laboratory of Atmospheric Physics, Aristotle University of Thessaloniki, Greece</affiliation>
		<affiliation numeration="2" content_type="html">Institute for Medical Physics, University of Innsbruck, Austria</affiliation>
	</affiliations>
	<abstract content_type="html">The results of two methods retrieving actinic flux and ozone photolysis
frequencies from measurements of irradiance with a Brewer MKIII
spectroradiometer are investigated in this paper. The first method uses
actinic flux retrieved from irradiance measurements by the use of known
formulas while the second is an empirical method converting irradiance to
ozone photolysis frequencies through polynomials extracted from a study of
synchronous actinic flux and irradiance measurements. When examining the
actinic fluxes derived from the first method to those measured by an actinic
flux spectrometer, data agree within &amp;plusmn;10% for solar zenith angles
lower than 75&amp;deg; for the UV-B and the UV-A wavelength band. Also, the
actinic to global irradiance ratio derived, deviates within &amp;plusmn;6% for
solar zenith angles lower than 70&amp;deg; compared with cloudless sky
calculations of the TUV model. For both cases the deviations are in the
order of the magnitude of the measurements or model uncertainties. The ozone
photolysis frequencies calculated by the second method show a mean ratio of
0.98&amp;plusmn;0.12 (1&amp;sigma; and 0.97&amp;plusmn;0.06 for all data and for
cloudless skies, respectively, when compared with ozone photolysis frequencies
derived by a Bentham actinic flux spectroradiometer. Finally, the agreement
of the two methods is within &amp;plusmn;5% comparing two years&apos; data of ozone
photolysis frequencies retrieved from irradiance measurements at
Thessaloniki, Greece. The use of such methods on extensive data sets of
global irradiance can provide JO&lt;sup&gt;1&lt;/sup&gt;D values with acceptable uncertainty, a parameter of particular importance for chemical process studies.</abstract>
	<references>
	</references>
</article>

