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<article language="en">
	<journal>
		<journal_title>Atmospheric Chemistry and Physics</journal_title>
		<journal_url>www.atmos-chem-phys.net</journal_url>
		<issn>1680-7316</issn>
		<eissn>1680-7324</eissn>
		<volume_number>9</volume_number>
		<issue_number>21</issue_number>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/acp-9-8283-2009</doi>
	<article_url>http://www.atmos-chem-phys.net/9/8283/2009/</article_url>
	<abstract_html>http://www.atmos-chem-phys.net/9/8283/2009/acp-9-8283-2009.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys.net/9/8283/2009/acp-9-8283-2009.pdf</fulltext_pdf>
	<start_page>8283</start_page>
	<end_page>8308</end_page>
	<publication_date>2009-11-03</publication_date>
	<article_title content_type="html">Observations of heterogeneous reactions between Asian pollution and mineral dust over the Eastern North Pacific during INTEX-B</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>C. S. McNaughton</name>
			<email>csmcnaug@hawaii.edu</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>A. D. Clarke</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>V. Kapustin</name>
		</author>
		<author numeration="4" affiliations="1,9">
			<name>Y. Shinozuka</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>S. G. Howell</name>
		</author>
		<author numeration="6" affiliations="2">
			<name>B. E. Anderson</name>
		</author>
		<author numeration="7" affiliations="2">
			<name>E. Winstead</name>
		</author>
		<author numeration="8" affiliations="3">
			<name>J. Dibb</name>
		</author>
		<author numeration="9" affiliations="3">
			<name>E. Scheuer</name>
		</author>
		<author numeration="10" affiliations="4">
			<name>R. C. Cohen</name>
		</author>
		<author numeration="11" affiliations="4">
			<name>P. Wooldridge</name>
		</author>
		<author numeration="12" affiliations="4">
			<name>A. Perring</name>
		</author>
		<author numeration="13" affiliations="5">
			<name>L. G. Huey</name>
		</author>
		<author numeration="14" affiliations="5">
			<name>S. Kim</name>
		</author>
		<author numeration="15" affiliations="6">
			<name>J. L. Jimenez</name>
		</author>
		<author numeration="16" affiliations="6">
			<name>E. J. Dunlea</name>
		</author>
		<author numeration="17" affiliations="6,10">
			<name>P. F. DeCarlo</name>
		</author>
		<author numeration="18" affiliations="7">
			<name>P. O. Wennberg</name>
		</author>
		<author numeration="19" affiliations="7">
			<name>J. D. Crounse</name>
		</author>
		<author numeration="20" affiliations="8">
			<name>A. J. Weinheimer</name>
		</author>
		<author numeration="21" affiliations="8">
			<name>F. Flocke</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">School of Ocean and Earth Science and Technology, University of Hawaii, Honolulu, 96822 HI, USA</affiliation>
		<affiliation numeration="2" content_type="html">NASA Langley Research Center, Hampton, 23665 VA, USA</affiliation>
		<affiliation numeration="3" content_type="html">University of New Hampshire, Durham, 03824 NH, USA</affiliation>
		<affiliation numeration="4" content_type="html">University of California Berkeley, Berkeley, 94720 CA, USA</affiliation>
		<affiliation numeration="5" content_type="html">Georgia Institute of Technology, Atlanta, 30332 GA, USA</affiliation>
		<affiliation numeration="6" content_type="html">Cooperative Institute for Research in Environmental Sciences (CIRES) and University of Colorado, Boulder, 80309 CO, USA</affiliation>
		<affiliation numeration="7" content_type="html">California Institute of Technology, Pasadena, 91125 CA, USA</affiliation>
		<affiliation numeration="8" content_type="html">National Center for Atmospheric Research, Boulder, 80307 CO, USA</affiliation>
		<affiliation numeration="9" content_type="html">now at: NASA Ames Research Center, Moffett Field, 94035 CA, USA</affiliation>
		<affiliation numeration="10" content_type="html">now at: Paul Scherrer Institute, 5232 Villigen-PSI, Switzerland</affiliation>
	</affiliations>
	<abstract content_type="html">In-situ airborne measurements of trace gases, aerosol size distributions,
chemistry and optical properties were conducted over Mexico and the Eastern
North Pacific during MILAGRO and INTEX-B. Heterogeneous reactions between
secondary aerosol precursor gases and mineral dust lead to sequestration of
sulfur, nitrogen and chlorine in the supermicrometer particulate size range.
&lt;br&gt;&lt;br&gt;
Simultaneous measurements of aerosol size distributions and weak-acid
soluble calcium result in an estimate of 11 wt% of CaCO&lt;sub&gt;3&lt;/sub&gt; for Asian
dust. During transport across the North Pacific, ~5â€“30% of the
CaCO&lt;sub&gt;3&lt;/sub&gt; is converted to CaSO&lt;sub&gt;4&lt;/sub&gt; or Ca(NO&lt;sub&gt;3&lt;/sub&gt;)&lt;sub&gt;2&lt;/sub&gt; with an
additional ~4% consumed through reactions with HCl. The 1996 to
2008 record from the Mauna Loa Observatory confirm these findings,
indicating that, on average, 19% of the CaCO&lt;sub&gt;3&lt;/sub&gt; has reacted to form
CaSO&lt;sub&gt;4&lt;/sub&gt; and 7% has reacted to form Ca(NO&lt;sub&gt;3&lt;/sub&gt;)&lt;sub&gt;2&lt;/sub&gt; and ~2%
has reacted with HCl. In the nitrogen-oxide rich boundary layer near Mexico
City up to 30% of the CaCO&lt;sub&gt;3&lt;/sub&gt; has reacted to form Ca(NO&lt;sub&gt;3&lt;/sub&gt;)&lt;sub&gt;2&lt;/sub&gt;
while an additional 8% has reacted with HCl.
&lt;br&gt;&lt;br&gt;
These heterogeneous reactions can result in a ~3% increase in dust
solubility which has an insignificant effect on their optical properties
compared to their variability in-situ. However, competition between
supermicrometer dust and submicrometer primary aerosol for condensing
secondary aerosol species led to a 25% smaller number median diameter for
the accumulation mode aerosol. A 10â€“25% reduction of accumulation mode
number median diameter results in a 30â€“70% reduction in submicrometer
light scattering at relative humidities in the 80â€“95% range. At 80% RH
submicrometer light scattering is only reduced ~3% due to a higher
mass fraction of hydrophobic refractory components in the dust-affected
accumulation mode aerosol. Thus reducing the geometric mean diameter of the
submicrometer aerosol has a much larger effect on aerosol optical properties
than changes to the hygroscopic:hydrophobic mass fractions of the
accumulation mode aerosol.
&lt;br&gt;&lt;br&gt;
In the presence of dust, nitric acid concentrations are reduced to &lt;50%
of total nitrate (nitric acid plus particulate nitrate). NO&lt;sub&gt;y&lt;/sub&gt; as a
fraction of total nitrogen (NO&lt;sub&gt;y&lt;/sub&gt; plus particulate nitrate), is reduced
from &gt;85% to 60â€“80% in the presence of dust. These observations
support previous model studies which predict irreversible sequestration of
reactive nitrogen species through heterogeneous reactions with mineral dust
during long-range transport.</abstract>
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</article>

