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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>2</volume_number>
		<issue_number>3</issue_number>
		<publication_year>2002</publication_year>
	</journal>
	<doi>10.5194/acpd-2-715-2002</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/2/715/2002/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/2/715/2002/acpd-2-715-2002.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/2/715/2002/acpd-2-715-2002.pdf</fulltext_pdf>
	<start_page>715</start_page>
	<end_page>738</end_page>
	<publication_date>2002-06-12</publication_date>
	<article_title content_type="html">Twilight tropospheric and stratospheric photodissociation rates derived from balloon borne radiation measurements</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>A. Kylling</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>T. Danielsen</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>M. Blumthaler</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>J. Schreder</name>
		</author>
		<author numeration="5" affiliations="3">
			<name>B. Johnsen</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Norwegian Institute for Air Research, Kjeller, Norway</affiliation>
		<affiliation numeration="2" content_type="html">Institute of Medical Physics, University of Innsbruck, Innsbruck, Austria</affiliation>
		<affiliation numeration="3" content_type="html">Norwegian Radiation Protection Authority, Oslo, Norway</affiliation>
	</affiliations>
	<abstract content_type="html">A new ligthweight multichannel moderate bandwidth filter instrument
      designed to be flown on balloons, is described. The instrument measures the radiation field within the short UV (center wavelength at
      312nm) and long UV (center wavelength at 340nm). The angular and spectral characteristics of the
      instrument are discussed and the calibration procedure outlined. Measurements made during a stratospheric balloon flight
      at twilight conditions from  Gap-Tallard, France, are presented and compared with state-of-the-art radiative transfer model
      simulations. The model simulations and the measurements agree within ±10%
      (±20%) for solar zenith angles smaller than 93° (90°) for the 340
      (312)nm channel. Based on the model simulations of the measured radiation,
      actinic flux spectra are reconstructed. These are used to calculate various photodissociation rates.</abstract>
	<references>
	</references>
</article>

