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<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" article-type="research-article" dtd-version="3.0" xml:lang="en">
<front>
<journal-meta>
<journal-id journal-id-type="publisher">ACPD</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics Discussions</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACPD</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7375</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acpd-6-8713-2006</article-id>
<title-group>
<article-title>Classification of aerosol properties derived from AERONET direct sun data</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Gobbi</surname>
<given-names>G. P.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kaufman</surname>
<given-names>Y. J.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Koren</surname>
<given-names>I.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Eck</surname>
<given-names>T. F.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Inst. Scienze dell’ Atmosfera e del Clima, CNR, Rome, Italy</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>NASA/Goddard Space Flight Center, 613.2, Greenbelt MD 20771, USA</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Dep. of Environ. Sciences Weizmann Institute, Rehovot 76100, Israel</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>GEST, University of Maryland, Baltimore, MD, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>14</day>
<month>09</month>
<year>2006</year>
</pub-date>
<volume>6</volume>
<issue>5</issue>
<fpage>8713</fpage>
<lpage>8726</lpage>
<permissions>
<license xlink:type="simple">
<license-p>This is an open-access article ditributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.</license-p>
</license>
</permissions>
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<self-uri xlink:href="http://www.atmos-chem-phys-discuss.net/6/8713/2006/acpd-6-8713-2006.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys-discuss.net/6/8713/2006/acpd-6-8713-2006.pdf</self-uri>
<abstract>
<p>Aerosol spectral measurements by sunphotometers can be characterized by
three independent pieces of information: 1) the optical thickness (AOT), a
measure of the column aerosol concentration, 2) the optical thickness
average spectral dependence, given by the Angstrom exponent (&amp;alpha;), and
3) the spectral curvature of &amp;alpha; (&amp;delta;&amp;alpha;). We propose a
simple graphical method to visually convert (&amp;alpha;, &amp;delta;&amp;alpha;)
to the contribution of fine aerosol to the AOT and the size of
the fine aerosols. This information can be used to track mixtures of
pollution aerosol with dust, to distinguish aerosol growth from cloud
contamination and to observe aerosol humidification. The graphical method is
applied to the analysis of yearly records at 8 sites in 3 continents,
characterized by different levels of pollution, biomass burning and mineral
dust concentrations. Results depict the dominance of fine mode aerosols in
driving the AOT at polluted sites. In stable meteorological conditions, we
see an increase in the size of the fine aerosol as the pollution stagnates
and increases in optical thickness. Coexistence of coarse and fine particles
is evidenced at the polluted sites downwind of arid regions.</p>
</abstract>
<counts><page-count count="14"/></counts>
</article-meta>
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