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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>2</volume_number>
		<issue_number>3</issue_number>
		<publication_year>2002</publication_year>
	</journal>
	<doi>10.5194/acpd-2-765-2002</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/2/765/2002/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/2/765/2002/acpd-2-765-2002.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/2/765/2002/acpd-2-765-2002.pdf</fulltext_pdf>
	<start_page>765</start_page>
	<end_page>788</end_page>
	<publication_date>2002-06-12</publication_date>
	<article_title content_type="html">The UV-visible absorption cross-sections of IONO&lt;sub&gt;2&lt;/sub&gt;</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J. C. Mössinger</name>
		</author>
		<author numeration="2" affiliations="1,2">
			<name>D. M. Rowley</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>R. A. Cox</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Centre for Atmospheric Science, Chemistry Department, University of Cambridge, UK</affiliation>
		<affiliation numeration="2" content_type="html">Present address Chemistry Department, University College London, UK</affiliation>
	</affiliations>
	<abstract content_type="html">The UV-visible absorption spectrum of gaseous
      IONO&lt;sub&gt;2&lt;/sub&gt; has been measured over the wavelength range 245--415 nm using the technique of laser photolysis with time-resolved
      UV-visible absorption spectroscopy. IONO&lt;sub&gt;2&lt;/sub&gt;
      was produced in situ in the gas phase by laser flash photolysis of NO&lt;sub&gt;2&lt;/sub&gt;/CF&lt;sub&gt;3&lt;/sub&gt;I/N&lt;sub&gt;2&lt;/sub&gt; mixtures. Post-flash spectra were deconvolved to
      remove contributions to the observed absorption from other reactant and product species.
      The resulting spectrum attributed to IONO&lt;sub&gt;2&lt;/sub&gt;
      consists of several overlapping broad absorption bands. Assuming a quantum yield of unity for
      IONO&lt;sub&gt;2&lt;/sub&gt;
      photolysis, model calculations show that during sunlit hours at noon, 53°
      N, the first order solar photolysis rate coefficient (J value) for IONO&lt;sub&gt;2&lt;/sub&gt;
      is 4.6 x 10&lt;sup&gt;-2&lt;/sup&gt; s&lt;sup&gt;-1&lt;/sup&gt;.</abstract>
	<references>
	</references>
</article>

