<?xml version="1.0" encoding="utf-8" standalone="no"?>
<!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>6</volume_number>
		<issue_number>3</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acpd-6-4251-2006</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/6/4251/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/6/4251/2006/acpd-6-4251-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/6/4251/2006/acpd-6-4251-2006.pdf</fulltext_pdf>
	<start_page>4251</start_page>
	<end_page>4272</end_page>
	<publication_date>2006-05-29</publication_date>
	<article_title content_type="html">MIPAS database: Validation of HNO&lt;sub&gt;3&lt;/sub&gt; line parameters using MIPAS satellite measurements</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J.-M. Flaud</name>
		</author>
		<author numeration="2" affiliations="2">
			<name>G. Brizzi</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>M. Carlotti</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>A. Perrin</name>
		</author>
		<author numeration="5" affiliations="2">
			<name>M. Ridolfi</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Laboratoire Interuniversitaire des Syst&amp;egrave;mes Atmosph&amp;eacute;riques (LISA), CNRS, Universit&amp;eacute;s Paris 12&amp;7, 61 avenue du G&amp;eacute;n&amp;eacute;ral de Gaulle, 94010 Cr&amp;eacute;teil Cedex, France</affiliation>
		<affiliation numeration="2" content_type="html">Dipartimento di Chimica Fisica e Inorganica, Universit&amp;agrave; di Bologna, Viale del Risorgimento, 4, 40136 Bologna, Italy</affiliation>
	</affiliations>
	<abstract content_type="html">Using new and accurate experimental results concerning
the spectroscopic properties of the HNO&lt;sub&gt;3&lt;/sub&gt; molecule as well as improved
theoretical methods it has been possible to generate an improved set of line
parameters for this molecule in the spectral range covered by the MIPAS
(&lt;B&gt;M&lt;/B&gt;ichelson &lt;B&gt;I&lt;/B&gt;nterferometer for &lt;B&gt;P&lt;/B&gt;assive
&lt;B&gt;A&lt;/B&gt;tmospheric &lt;B&gt;S&lt;/B&gt;ounding) experiment. These line parameters,
which have been validated using broadband atmospheric spectra recorded by
MIPAS, have been included in the last version of the MIPAS spectroscopic
database to be used for future processing of the MIPAS spectra.</abstract>
	<references>
	</references>
</article>

