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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>10</volume_number>
		<issue_number>3</issue_number>
		<publication_year>2010</publication_year>
	</journal>
	<doi>10.5194/acpd-10-6279-2010</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/10/6279/2010/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/10/6279/2010/acpd-10-6279-2010.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/10/6279/2010/acpd-10-6279-2010.pdf</fulltext_pdf>
	<start_page>6279</start_page>
	<end_page>6300</end_page>
	<publication_date>2010-03-08</publication_date>
	<article_title content_type="html">Brown carbon in tar balls from smoldering biomass combustion</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>R. K. Chakrabarty</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>H. Moosmüller</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>L.-W. A. Chen</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>K. Lewis</name>
		</author>
		<author numeration="5" affiliations="2">
			<name>W. P. Arnott</name>
		</author>
		<author numeration="6" affiliations="3,4">
			<name>C. Mazzolen</name>
		</author>
		<author numeration="7" affiliations="4">
			<name>M. Dubey</name>
		</author>
		<author numeration="8" affiliations="5">
			<name>C. E. Wold</name>
		</author>
		<author numeration="9" affiliations="5">
			<name>W. M. Hao</name>
		</author>
		<author numeration="10" affiliations="6">
			<name>S. M. Kreidenweis</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Division of Atmospheric Sciences, Desert Research Institute, Reno, NV 89512, USA</affiliation>
		<affiliation numeration="2" content_type="html">Department of Physics, University of Nevada, Reno, NV 89557, USA</affiliation>
		<affiliation numeration="3" content_type="html">Department of Physics, Michigan Technological University, MI 49931, USA</affiliation>
		<affiliation numeration="4" content_type="html">Geochemistry and Climate Focus Team, Los Alamos National Laboratory, NM 87547, USA</affiliation>
		<affiliation numeration="5" content_type="html">Fire Sciences Laboratory, USDA Forest Service, Missoula, MT 59808, USA</affiliation>
		<affiliation numeration="6" content_type="html">Department of Atmospheric Sciences, Colorado State University, CO 80523, USA</affiliation>
	</affiliations>
	<abstract content_type="html">We report the direct observation of large-scale production of spherical,
carbonaceous particles – &quot;tar balls&quot; – from smoldering combustion of two
commonly occurring dry mid-latitude fuels. Real-time measurements indicate
that brown carbon is an important component of tar balls. The spectrum of
the imaginary parts of their complex refractive indices can be described
with a Lorentzian-like model with an effective resonance wavelength in the
ultraviolet (UV) spectral region. Sensitivity calculations for
aerosols containing traditional organic carbon (no absorption at visible and
UV wavelengths) and brown carbon suggest that accounting for UV absorption
by brown carbon leads to a significant increase in aerosol radiative forcing
efficiency and increased atmospheric warming. Since particles from
smoldering combustion account for nearly three-fourths of the total
carbonaceous aerosol mass emitted globally, inclusion of the optical
properties of tar balls into radiative forcing models has significance for
the Earth&apos;s radiation budget, optical remote sensing, and understanding of
anomalous UV absorption in the troposphere.</abstract>
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</article>

