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<article language="en">
	<journal>
		<journal_title>Atmospheric Measurement Techniques Discussions</journal_title>
		<journal_url>www.atmos-meas-tech-discuss.net</journal_url>
		<eissn>1867-8610</eissn>
		<volume_number>3</volume_number>
		<issue_number>2</issue_number>
		<publication_year>2010</publication_year>
	</journal>
	<doi>10.5194/amtd-3-863-2010</doi>
	<article_url>http://www.atmos-meas-tech-discuss.net/3/863/2010/</article_url>
	<abstract_html>http://www.atmos-meas-tech-discuss.net/3/863/2010/amtd-3-863-2010.html</abstract_html>
	<fulltext_pdf>http://www.atmos-meas-tech-discuss.net/3/863/2010/amtd-3-863-2010.pdf</fulltext_pdf>
	<start_page>863</start_page>
	<end_page>889</end_page>
	<publication_date>2010-03-03</publication_date>
	<article_title content_type="html">Novel SO&lt;sub&gt;2&lt;/sub&gt; spectral evaluation scheme using the 360&amp;ndash;390 nm wavelength range</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>N. Bobrowski</name>
			<email>n.bobrowski@iup.uni-heidelberg.de</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>C. Kern</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>U. Platt</name>
		</author>
		<author numeration="4" affiliations="1,2">
			<name>C. HÃ¶rmann</name>
		</author>
		<author numeration="5" affiliations="2">
			<name>T. Wagner</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institute for Environmental Physics, University of Heidelberg, Germany</affiliation>
		<affiliation numeration="2" content_type="html">Max-Planck Institute for Chemistry, Mainz, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">Differential Optical Absorption Spectroscopy (DOAS) is a well established spectroscopic
      method to determine trace gases in the atmosphere. During the last decade, passive DOAS,
      which uses solar radiation scattered in the atmosphere as a light source, has become
      a standard tool to determine SO&lt;sub&gt;2&lt;/sub&gt; column densities and emission fluxes from volcanoes
      and other large sources by ground based as well as satellite measurements. For the
      determination of SO&lt;sub&gt;2&lt;/sub&gt; column densities, the structured absorption of the molecule in
      the 300â€“330 nm region (due to the A&lt;sup&gt;1&lt;/sup&gt;B&lt;sub&gt;1&lt;/sub&gt;&amp;larr;X&lt;sup&gt;1&lt;/sup&gt;A&lt;sub&gt;1&lt;/sub&gt;
      transition) is used. However, there are several problems limiting the accuracy of the
      technique in this particular application. Here we propose to use an alternative wavelength
      region (360â€“390 nm) due to the spin-forbidden a&lt;sup&gt;3&lt;/sup&gt;B&lt;sub&gt;2&lt;/sub&gt;&amp;larr;X&lt;sup&gt;1&lt;/sup&gt;A&lt;sub&gt;1&lt;/sub&gt; 
transition for the DOAS evaluation of SO&lt;sub&gt;2&lt;/sub&gt; in conditions where
      high SO&lt;sub&gt;2&lt;/sub&gt; column densities prevail. We show this range to have considerable
      advantages in such cases, in particular when the particle content of the plume is high and
      when measurements are performed at large distances from the area of interest.</abstract>
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