<?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>6</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acpd-6-11597-2006</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/6/11597/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/6/11597/2006/acpd-6-11597-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/6/11597/2006/acpd-6-11597-2006.pdf</fulltext_pdf>
	<start_page>11597</start_page>
	<end_page>11620</end_page>
	<publication_date>2006-11-20</publication_date>
	<article_title content_type="html">Near-UV photolysis cross sections of CH&lt;sub&gt;3&lt;/sub&gt;OOH and HOCH&lt;sub&gt;2&lt;/sub&gt;OOH determined via action spectroscopy</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>C. M. Roehl</name>
		</author>
		<author numeration="2" affiliations="1,4">
			<name>Z. Marka</name>
		</author>
		<author numeration="3" affiliations="2,5">
			<name>J. L. Fry</name>
		</author>
		<author numeration="4" affiliations="1,3">
			<name>P. O. Wennberg</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA</affiliation>
		<affiliation numeration="2" content_type="html">Arthur Amos Noyes Laboratory of Chemical Physics, California Institute of Technology, Pasadena, CA 91125, USA</affiliation>
		<affiliation numeration="3" content_type="html">Division of Engineering and Applied Science, California Institute of Technology, Pasadena, CA 91125, USA</affiliation>
		<affiliation numeration="4" content_type="html">now at: Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA</affiliation>
		<affiliation numeration="5" content_type="html">now at: Department of Chemistry, University of California, Berkeley, Berkeley, CA 94720-1460, USA</affiliation>
	</affiliations>
	<abstract content_type="html">Knowledge of molecular photolysis cross sections is important for
determining atmospheric lifetimes and fates of many species. A method and
laser apparatus for measurement of these cross sections in the
near-ultraviolet (UV) region is described. The technique is based on action
spectroscopy, where the yield of a photodissociation product (in this case
OH) is measured as a function of excitation energy. For compounds yielding
OH, this method can be used to measure near-UV photodissociation cross
section as low as 10&lt;sup&gt;&amp;minus;23&lt;/sup&gt; cm&lt;sup&gt;2&lt;/sup&gt; molecule&lt;sup&gt;&amp;minus;1&lt;/sup&gt;. The method is applied
to determine the photodissociation cross sections for methyl hydroperoxide
(CH&lt;sub&gt;3&lt;/sub&gt;OOH; MHP) and hydroxymethyl hydroperoxide (HOCH&lt;sub&gt;2&lt;/sub&gt;OOH; HMHP) in
the 305&amp;ndash;365 nm wavelength range. The measured cross sections are in good
agreement with previous measurements of absorption cross sections.</abstract>
	<references>
	</references>
</article>

