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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>5</issue_number>
		<publication_year>2004</publication_year>
	</journal>
	<doi>10.5194/acpd-4-5655-2004</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/4/5655/2004/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/4/5655/2004/acpd-4-5655-2004.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/4/5655/2004/acpd-4-5655-2004.pdf</fulltext_pdf>
	<start_page>5655</start_page>
	<end_page>5681</end_page>
	<publication_date>2004-09-22</publication_date>
	<article_title content_type="html">High resolution mid-infrared cross-sections for peroxyacetyl nitrate (PAN) vapour</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>G. Allen</name>
			<email>ga15@le.ac.uk</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>J. J. Remedios</name>
		</author>
		<author numeration="3" affiliations="2,4">
			<name>D. A. Newnham</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>K. M. Smith</name>
		</author>
		<author numeration="5" affiliations="3">
			<name>P. S. Monks</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">EOS, Space Research Centre, Dept. of Physics and Astronomy, Univ. Leicester, Leicester, LE1 7RH, UK</affiliation>
		<affiliation numeration="2" content_type="html">Space Science &amp; Technology Dept., Rutherford Appleton Lab., Didcot, Oxon, OX11 0QX, UK</affiliation>
		<affiliation numeration="3" content_type="html">Department of Chemistry, Univ. Leicester, Leicester, LE1 7RH, UK</affiliation>
		<affiliation numeration="4" content_type="html">now at: TeraView Limited, 302/304 Science Park, Milton Road, Cambridge, CB4 0WG, UK</affiliation>
	</affiliations>
	<abstract content_type="html">Absorption spectra of peroxyacetyl nitrate (PAN, CH&lt;sub&gt;3&lt;/sub&gt;C(O)OONO&lt;sub&gt;2&lt;/sub&gt;)
vapour at room temperature (295 K) have been measured in the mid-infrared
range, 550&amp;ndash;2200 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt; (18.2&amp;ndash;3.33 &amp;micro;m), using a Fourier transform
infrared spectrometer at instrument resolutions of 0.25 and 0.03 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt;
(unapodised). Both cross-section data and integrated absorption intensities
for the five principal bands in the PAN spectra in this spectral range have
been derived from fourteen separate PAN transmission spectra measurements.
Band intensities and band centre absorptivities are also reported for four
weaker PAN absorption bands in the mid infrared for the first time. These
observations are the highest spectral resolution measurements of PAN bands
recorded in the infrared to date. For three of the five strongest bands, the
absolute integrated absorption intensities are in excellent agreement with
previous studies. A 4.8% lower integrated intensity was found for the
1741 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt; &amp;nu;&lt;sub&gt;&lt;i&gt;as&lt;/i&gt;&lt;/sub&gt; (NO&lt;sub&gt;2&lt;/sub&gt;) PAN absorption band, possibly as a
result of the removal in this work of spectra affected by subtle acetone
contamination, while a 10.6% higher intensity was determined for the 1163 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt; &amp;nu; (C-O) 
absorption band. No direct effects of spectral
resolution were observed. The improved accuracy of these absorption
cross-sections will allow more accurate investigations of PAN using infrared
spectroscopy, particularly for remote sensing of PAN in the atmosphere.</abstract>
	<references>
	</references>
</article>

