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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>7</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2007</publication_year>
	</journal>
	<doi>10.5194/acpd-7-10065-2007</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/7/10065/2007/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/7/10065/2007/acpd-7-10065-2007.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/7/10065/2007/acpd-7-10065-2007.pdf</fulltext_pdf>
	<start_page>10065</start_page>
	<end_page>10096</end_page>
	<publication_date>2007-07-11</publication_date>
	<article_title content_type="html">Evolving mass spectra of the oxidized component of organic aerosol: results from aerosol mass spectrometer analyses of aged diesel emissions</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>A. M. Sage</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>E. A. Weitkamp</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>A. L. Robinson</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>N. M. Donahue</name>
			<email>nmd@.cmu.edu</email>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Center for Atmospheric Particle Studies, Carnegie Mellon University; Pittsburgh, PA  15213, USA</affiliation>
	</affiliations>
	<abstract content_type="html">The species and chemistry responsible for secondary organic aerosol
(SOA) formation remain highly uncertain. Laboratory studies of the oxidation
of individual, high-flux SOA precursors do not lead to particles with mass
spectra (MS) matching those of ambient aged organic material. And, the
complexity of real organic particles challenges efforts to identify their
chemical origins. We have previously hypothesized that SOA can form from the
atmospheric oxidation of a large suite of precursors with varying vapor
pressures. Here, we support this hypothesis by using an aerosol mass
spectrometer to track the chemical evolution of diesel exhaust as it is
photochemically oxidized in an environmental chamber. With explicit knowledge
of the condensed-phase MS of the primary emissions from our
engine, we are able to decompose each recorded MS into
contributing primary and secondary spectra throughout the experiment. We find
that the SOA MS becomes increasingly oxidized as a function of time,
eventually reaching a final MS that closely resembles that of ambient aged
organic particulate matter. This observation is consistent with the idea that
lower vapor pressure, semi-volatile organic emissions can form condensable
products with fewer generations of oxidation, and therefore, they form
relatively less oxidized SOA very quickly.</abstract>
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</article>

