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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>3</issue_number>
		<publication_year>2008</publication_year>
	</journal>
	<doi>10.5194/acpd-8-10189-2008</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/8/10189/2008/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/8/10189/2008/acpd-8-10189-2008.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/8/10189/2008/acpd-8-10189-2008.pdf</fulltext_pdf>
	<start_page>10189</start_page>
	<end_page>10225</end_page>
	<publication_date>2008-05-30</publication_date>
	<article_title content_type="html">Estimation of the mass absorption cross section of the organic carbon component of aerosols in the Mexico City Metropolitan Area (MCMA)</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J. C. Barnard</name>
			<email>james.barnard@pnl.gov</email>
		</author>
		<author numeration="2" affiliations="2">
			<name>R. Volkamer</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>E. I. Kassianov</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Pacific Northwest National Laboratory, Richland, WA, USA</affiliation>
		<affiliation numeration="2" content_type="html">University of Colorado, Boulder, CO, USA</affiliation>
	</affiliations>
	<abstract content_type="html">Data taken from the MCMA-2003 and the 2006 MILAGRO field campaigns are used
to examine the absorption of solar radiation by the organic component of
aerosols. Using irradiance data from a Multi-Filter Rotating Shadowband
Radiometer (MFRSR) and an actinic flux spectroradiometer (SR), we derive
aerosol single scattering albedo, &amp;pi;&lt;sub&gt;0,&amp;lambda;&lt;/sub&gt;, as a function of
wavelength, λ. We find that in the near-UV spectral range (250 to 400 nm)
&amp;pi;&lt;sub&gt;0,&amp;lambda;&lt;/sub&gt; is much lower compared to &amp;pi;&lt;sub&gt;0,&amp;lambda;&lt;/sub&gt; at 500 nm
indicating enhanced absorption in the near-UV range. Absorption by elemental
carbon, dust, or gas cannot account for this enhanced absorption leaving the
organic part of the aerosol as the only possible absorber. We use data from
a surface deployed Aerodyne Aerosol Mass Spectrometer (AMS) along with the
inferred &amp;pi;&lt;sub&gt;0,&amp;lambda;&lt;/sub&gt; to estimate the Mass Absorption Cross section (MAC)
for the organic carbon. We find that the MAC is about 10.5 m&lt;sup&gt;2&lt;/sup&gt;/g at 300 nm and falls close to zero at about 500 nm; values that are roughly
consistent with other estimates of organic carbon MAC. These MAC values can
be considered as &quot;radiatively correct&quot; because when used in radiative
transfer calculations the calculated irradiances/actinic fluxes match those
measured at the wavelengths considered here. For an illustrative case study
described here, we estimate that the light absorption by the &quot;brown&quot;
(organic) carbonaceous aerosol can add about 40% to the light absorption
of black carbon in Mexico City. This contribution will vary depending on the
relative abundance of organic carbon relative to black carbon. Furthermore,
our analysis indicates that organic aerosol would slow down photochemistry
by selectively scavenging the light reaching the ground at those wavelengths
that drive photochemical reactions. Finally, satellite retrievals of trace
gases that are used to infer emissions currently assume that the MAC of
organic carbon is zero. For trace gases that are retrieved using wavelengths
shorter then 420 nm (i.e. SO&lt;sub&gt;2&lt;/sub&gt;, HCHO, halogenoxides, NO&lt;sub&gt;2&lt;/sub&gt;), the
assumption of non-zero MAC values will induce an upward correction to the
inferred emissions. This will be particularly relevant in polluted urban
atmospheres and areas of biomass burning where organic aerosols are
particularly abundant.</abstract>
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</article>

