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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>8</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2008</publication_year>
	</journal>
	<doi>10.5194/acpd-8-15343-2008</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/8/15343/2008/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/8/15343/2008/acpd-8-15343-2008.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/8/15343/2008/acpd-8-15343-2008.pdf</fulltext_pdf>
	<start_page>15343</start_page>
	<end_page>15373</end_page>
	<publication_date>2008-08-13</publication_date>
	<article_title content_type="html">Loading-dependent elemental composition of &amp;alpha;-pinene SOA particles</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J. E. Shilling</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>Q. Chen</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>S. M. King</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>T. Rosenoern</name>
		</author>
		<author numeration="5" affiliations="2">
			<name>J. H. Kroll</name>
		</author>
		<author numeration="6" affiliations="2">
			<name>D. R. Worsnop</name>
		</author>
		<author numeration="7" affiliations="3,4,7">
			<name>P. F. DeCarlo</name>
		</author>
		<author numeration="8" affiliations="4,5">
			<name>A. C. Aiken</name>
		</author>
		<author numeration="9" affiliations="2,4,5">
			<name>D. Sueper</name>
		</author>
		<author numeration="10" affiliations="4,5">
			<name>J. L. Jimenez</name>
		</author>
		<author numeration="11" affiliations="1,6">
			<name>S. T. Martin</name>
			<email>scot_martin@harvard.edu</email>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">School of Engineering and Applied Sciences, Harvard University, Cambridge, MA 02138, USA</affiliation>
		<affiliation numeration="2" content_type="html">Aerodyne Research, Inc., Billerica, MA 08121, USA</affiliation>
		<affiliation numeration="3" content_type="html">Department of Atmospheric and Oceanic Sciences University of Colorado, Boulder, CO 80309, USA</affiliation>
		<affiliation numeration="4" content_type="html">Cooperative Institute for Research in the Environmental Sciences (CIRES), University of Colorado, Boulder, CO 80309, USA</affiliation>
		<affiliation numeration="5" content_type="html">Department of Chemistry and Biochemistry, University of Colorado, Boulder, CO 80309, USA</affiliation>
		<affiliation numeration="6" content_type="html">Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA 02138, USA</affiliation>
		<affiliation numeration="7" content_type="html">now at: Paul Scherrer Institut, Laboratory of Atmospheric Chemistry, Villigen-PSI, 5232, Switzerland</affiliation>
	</affiliations>
	<abstract content_type="html">The chemical composition of secondary organic aerosol (SOA) particles,
formed by the dark ozonolysis of α-pinene, was characterized by a
high-resolution time-of-flight aerosol mass spectrometer. The experiments
were conducted using a continuous-flow chamber, allowing the particle mass
loading and chemical composition to be maintained for several days. The
organic portion of the particle mass loading was varied from 0.5 to
&amp;gt;140 μg/m&lt;sup&gt;3&lt;/sup&gt; by adjusting the concentration of reacted &amp;alpha;-pinene
from 0.9 to 91.1 ppbv. The mass spectra of the organic material changed with
loading. For loadings below 5 μg/m&lt;sup&gt;3&lt;/sup&gt; the unit-mass-resolution
&lt;i&gt;m/z&lt;/i&gt; 44 signal intensity exceeded that of &lt;i&gt;m/z&lt;/i&gt; 43, suggesting more oxygenated
organic material at lower loadings. Composition measurements displayed a
greater dependence for lower loadings (0.5 to 15 μg/m&lt;sup&gt;3&lt;/sup&gt;) compared
to higher loadings (15 to &amp;gt;140 μg/m&lt;sup&gt;3&lt;/sup&gt;). The high-resolution mass
spectra showed that from &amp;gt;140 to 0.5 μg/m&lt;sup&gt;3&lt;/sup&gt; the mass percentage
of fragments containing carbon and oxygen (C&lt;sub&gt;x&lt;/sub&gt;H&lt;sub&gt;y&lt;/sub&gt;O&lt;sub&gt;z&lt;/sub&gt;&lt;sup&gt;+&lt;/sup&gt;)
monotonically increased from 48% to 54%. Correspondingly, the mass
percentage of fragments representing C&lt;sub&gt;x&lt;/sub&gt;H&lt;sub&gt;y&lt;/sub&gt;&lt;sup&gt;+&lt;/sup&gt; decreased from
52% to 46%, and the atomic oxygen-to-carbon ratio increased from 0.29
to 0.45. The atomic ratios were accurately parameterized by a four-product
basis set of decadal volatility (viz. 0.1, 1.0, 10, 100 μg/m&lt;sup&gt;&amp;minus;3&lt;/sup&gt;)
employing products with the empirical formulas C&lt;sub&gt;1&lt;/sub&gt;H&lt;sub&gt;1.32&lt;/sub&gt;O&lt;sub&gt;0.48&lt;/sub&gt;,
C&lt;sub&gt;1&lt;/sub&gt;H&lt;sub&gt;1.36&lt;/sub&gt;O&lt;sub&gt;0.39&lt;/sub&gt;, C&lt;sub&gt;1&lt;/sub&gt;H&lt;sub&gt;1.57&lt;/sub&gt;O&lt;sub&gt;0.24&lt;/sub&gt;, and
C&lt;sub&gt;1&lt;/sub&gt;H&lt;sub&gt;1.76&lt;/sub&gt;O&lt;sub&gt;0.14&lt;/sub&gt;. These findings suggest considerable caution is
warranted in the extrapolation of laboratory results that were obtained
under conditions of relatively high loading (i.e., &amp;gt;15 μg/m&lt;sup&gt;3&lt;/sup&gt;) to
modeling applications relevant to the atmosphere, for which loadings of 0.1
to 20 μg/m&lt;sup&gt;3&lt;/sup&gt; are typical. For the lowest loadings, the particle
mass spectra resembled observations reported in the literature for some
atmospheric particles.</abstract>
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