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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>3</volume_number>
		<issue_number>6</issue_number>
		<publication_year>2003</publication_year>
	</journal>
	<doi>10.5194/acpd-3-5689-2003</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/3/5689/2003/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/3/5689/2003/acpd-3-5689-2003.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/3/5689/2003/acpd-3-5689-2003.pdf</fulltext_pdf>
	<start_page>5689</start_page>
	<end_page>5710</end_page>
	<publication_date>2003-11-12</publication_date>
	<article_title content_type="html">Measurements of the sum of HO&lt;sub&gt;2&lt;/sub&gt;NO&lt;sub&gt;2&lt;/sub&gt; and CH&lt;sub&gt;3&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt;NO&lt;sub&gt;2&lt;/sub&gt; in the remote troposphere</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J. G. Murphy</name>
		</author>
		<author numeration="2" affiliations="1,5">
			<name>J. A. Thornton</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>P. J. Wooldridge</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>D. A. Day</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>R. S. Rosen</name>
		</author>
		<author numeration="6" affiliations="2">
			<name>C. Cantrell</name>
		</author>
		<author numeration="7" affiliations="2">
			<name>R. E. Shetter</name>
		</author>
		<author numeration="8" affiliations="2">
			<name>B. Lefer</name>
		</author>
		<author numeration="9" affiliations="1,3,4">
			<name>R. C. Cohen</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">University of California at Berkeley, Department of Chemistry, Berkeley, CA, USA</affiliation>
		<affiliation numeration="2" content_type="html">National Center for Atmospheric Research, Atmospheric Chemistry Division, Boulder, CO, USA</affiliation>
		<affiliation numeration="3" content_type="html">University of California at Berkeley, Department of Earth and Planetary Science, Berkeley, CA, USA</affiliation>
		<affiliation numeration="4" content_type="html">Lawrence Berkeley National Laboratory, Division of Energy and Environment Technologies, Berkeley, CA, USA</affiliation>
		<affiliation numeration="5" content_type="html">now at University of Toronto, Department of Chemistry, Toronto, ON, Canada</affiliation>
	</affiliations>
	<abstract content_type="html">The chemistry of peroxynitric acid (HO&lt;sub&gt;2&lt;/sub&gt;NO&lt;sub&gt;2&lt;/sub&gt;) and methyl peroxynitrate
      (CH&lt;sub&gt;3&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt;NO&lt;sub&gt;2&lt;/sub&gt;) is
      predicted to be particularly important in the upper troposphere where temperatures are
      frequently low enough that these compounds do not rapidly decompose. At temperatures
      below 240 K, we calculate that about 20% of NO&lt;sub&gt;y&lt;/sub&gt; in the mid and polar latitude upper
      troposphere is HO&lt;sub&gt;2&lt;/sub&gt;NO&lt;sub&gt;2&lt;/sub&gt;. Under these conditions, the reaction of OH with
      HO&lt;sub&gt;2&lt;/sub&gt;NO&lt;sub&gt;2&lt;/sub&gt; is
      estimated to account for as much as one third of the permanent loss of hydrogen radicals.
      During the Tropospheric Ozone Production about the Spring Equinox (TOPSE) campaign, we used thermal dissociation laser-induced fluorescence (TD-LIF) to measure
      the sum of peroxynitrates (&lt;font face=&quot;Symbol&quot;&gt;S&lt;/font&gt;PNs equivanlent HO&lt;sub&gt;2&lt;/sub&gt;NO&lt;sub&gt;2&lt;/sub&gt; +
      CH&lt;sub&gt;3&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt;NO&lt;sub&gt;2&lt;/sub&gt; + PAN + PPN + ...), aboard
      the NCAR C-130 research aircraft.  We infer the sum of HO&lt;sub&gt;2&lt;/sub&gt;NO&lt;sub&gt;2&lt;/sub&gt; and
      CH&lt;sub&gt;3&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt;NO&lt;sub&gt;2&lt;/sub&gt; as the
      difference between &lt;font face=&quot;Symbol&quot;&gt;S&lt;/font&gt;PN measurements and gas chromatographic measurements of the
      two major peroxy acyl nitrates, peroxy acetyl nitrate (PAN) and peroxy propionyl nitrate
      (PPN). Comparison with NO&lt;sub&gt;y&lt;/sub&gt; and other nitrogen oxide measurements confirms the
      importance of HO&lt;sub&gt;2&lt;/sub&gt;NO&lt;sub&gt;2&lt;/sub&gt; and
      CH&lt;sub&gt;3&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt;NO&lt;sub&gt;2&lt;/sub&gt; to the reactive nitrogen budget and shows that
      current thinking about the chemistry of these species is approximately correct.  The
      temperature dependence of the inferred concentrations corroborates the contribution of
      overtone photolysis to the photochemistry of peroxynitric acid.</abstract>
	<references>
	</references>
</article>

