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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>9</volume_number>
		<issue_number>6</issue_number>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/acpd-9-27745-2009</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/9/27745/2009/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/9/27745/2009/acpd-9-27745-2009.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/9/27745/2009/acpd-9-27745-2009.pdf</fulltext_pdf>
	<start_page>27745</start_page>
	<end_page>27789</end_page>
	<publication_date>2009-12-23</publication_date>
	<article_title content_type="html">Organic aerosol components observed in worldwide datasets from aerosol mass spectrometry</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>N. L. Ng</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>M. R. Canagaratna</name>
			<email>mrcana@aerodyne.com</email>
		</author>
		<author numeration="3" affiliations="2,12">
			<name>Q. Zhang</name>
		</author>
		<author numeration="4" affiliations="3,4">
			<name>J. L. Jimenez</name>
		</author>
		<author numeration="5" affiliations="2">
			<name>J. Tian</name>
		</author>
		<author numeration="6" affiliations="3,4">
			<name>I. M. Ulbrich</name>
		</author>
		<author numeration="7" affiliations="1,5">
			<name>J. H. Kroll</name>
		</author>
		<author numeration="8" affiliations="3,4">
			<name>K. S. Docherty</name>
		</author>
		<author numeration="9" affiliations="6">
			<name>P. S. Chhabra</name>
		</author>
		<author numeration="10" affiliations="3,7">
			<name>R. Bahreini</name>
		</author>
		<author numeration="11" affiliations="7">
			<name>S. M. Murphy</name>
		</author>
		<author numeration="12" affiliations="6">
			<name>J. H. Seinfeld</name>
		</author>
		<author numeration="13" affiliations="8">
			<name>L. Hildebrandt</name>
		</author>
		<author numeration="14" affiliations="3,9,10">
			<name>P. F. DeCarlo</name>
		</author>
		<author numeration="15" affiliations="10">
			<name>V. A. Lanz</name>
		</author>
		<author numeration="16" affiliations="10">
			<name>A. S. H. Prevot</name>
		</author>
		<author numeration="17" affiliations="11">
			<name>E. Dinar</name>
		</author>
		<author numeration="18" affiliations="11">
			<name>Y. Rudich</name>
		</author>
		<author numeration="19" affiliations="1">
			<name>D. R. Worsnop</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Aerodyne Research, Inc. Billerica, MA, USA</affiliation>
		<affiliation numeration="2" content_type="html">Atmospheric Sciences Research Center, State University of New York, Albany, NY, USA</affiliation>
		<affiliation numeration="3" content_type="html">CIRES, University of Colorado, Boulder, CO, USA</affiliation>
		<affiliation numeration="4" content_type="html">Department of Chemistry and Biochemistry, University of Colorado, Boulder, CO, USA</affiliation>
		<affiliation numeration="5" content_type="html">Department of Civil and Environmental Engineering, Massachusetts Institute of Technology, Cambridge, MA, USA</affiliation>
		<affiliation numeration="6" content_type="html">Department of Chemical Engineering, California Institute of Technology, Pasadena, CA, USA</affiliation>
		<affiliation numeration="7" content_type="html">NOAA, Earth System Research Laboratory, Boulder, CO, USA</affiliation>
		<affiliation numeration="8" content_type="html">Center for Atmospheric Particle Studies, Carnegie Mellon University, Pittsburgh, PA, USA</affiliation>
		<affiliation numeration="9" content_type="html">Department of Atmospheric and Oceanic Science, University of Colorado, Boulder, CO, USA</affiliation>
		<affiliation numeration="10" content_type="html">Laboratory of Atmospheric Chemistry, Paul Scherrer Institut, Villigen, Switzerland</affiliation>
		<affiliation numeration="11" content_type="html">Department of Environmental Sciences, Weizmann Institute of Science, Rehovot 76100, Israel</affiliation>
		<affiliation numeration="12" content_type="html">now at: Department of Environmental Toxicology, University of California, Davis, CA, USA</affiliation>
	</affiliations>
	<abstract content_type="html">In this study we present results from the factor analysis of 43
      aerosol mass spectrometer (AMS) datasets and provide an overview of
      worldwide organic aerosol (OA) components and their evolution in the
      atmosphere. At most sites, the OA can be separated into oxygenated OA
      (OOA), hydrocarbon-like OA (HOA), and sometimes other components such
      as biomass burning OA (BBOA). In many analyses, the OOA can be further
      deconvolved into low-volatility OOA (LV-OOA) and semi-volatile OOA
      (SV-OOA). A wide range of &lt;i&gt;f&lt;/i&gt;&lt;sub&gt;44&lt;/sub&gt; (ratio of &lt;i&gt;m/z&lt;/i&gt; 44 to
      total signal in the component mass spectrum) and O:C ratios are
      observed for both LV-OOA (0.17&amp;plusmn;0.04, 0.73&amp;plusmn;0.14) and SV-OOA
      (0.07&amp;plusmn;0.04, 0.35&amp;plusmn;0.14) components, reflecting the fact
      that there is a continuum of OOA properties in ambient
      aerosol. Differences in the mass spectra of these components are
      characterized in terms of the two main ions &lt;i&gt;m/z&lt;/i&gt; 44
      (CO&lt;sub&gt;2&lt;/sub&gt;&lt;sup&gt;+&lt;/sup&gt;) and &lt;i&gt;m/z&lt;/i&gt; 43 (mostly
      C&lt;sub&gt;2&lt;/sub&gt;H&lt;sub&gt;3&lt;/sub&gt;O&lt;sup&gt;+&lt;/sup&gt;). The LV-OOA component spectra have higher &lt;i&gt;f&lt;/i&gt;&lt;sub&gt;44&lt;/sub&gt;
      and lower &lt;i&gt;f&lt;/i&gt;&lt;sub&gt;43&lt;/sub&gt; than SV-OOA. The OOA components (OOA, LV-OOA, and
      SV-OOA) from all sites cluster within a well defined triangular region
      in the &lt;i&gt;f&lt;/i&gt;&lt;sub&gt;44&lt;/sub&gt; vs. &lt;i&gt;f&lt;/i&gt;&lt;sub&gt;43&lt;/sub&gt; space, which can be used as
      a standardized means of comparing and characterizing any OOA
      components (laboratory or ambient) observed with the AMS. Examination
      of the OOA components in this triangular space indicates that OOA
      component spectra become increasingly similar to each other and to
      fulvic acid and HULIS sample spectra as &lt;i&gt;f&lt;/i&gt;&lt;sub&gt;44&lt;/sub&gt; (a surrogate for O:C
      and an indicator of photochemical aging) increases. This indicates
      that ambient OA converges towards highly aged LV-OOA with atmospheric
      oxidation. The common features of the transformation between SV-OOA
      and LV-OOA at multiple sites potentially enables a simplified
      description of the oxidation of OA in the atmosphere. Comparison of
      laboratory SOA data with ambient OOA indicates that laboratory SOA are
      more similar to SV-OOA, and rarely become as oxidized as ambient
      LV-OOA, likely due to the higher loadings employed in the experiments
      and/or limited oxidant exposure in most chamber experiments.</abstract>
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</article>

