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<!DOCTYPE article SYSTEM "http://www.atmos-chem-phys-discuss.net/inc/acpd/copernicus.dtd">
<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>5</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/acpd-5-4929-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/4929/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/4929/2005/acpd-5-4929-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/4929/2005/acpd-5-4929-2005.pdf</fulltext_pdf>
	<start_page>4929</start_page>
	<end_page>4969</end_page>
	<publication_date>2005-07-14</publication_date>
	<article_title content_type="html">Aerosol optical properties at Lampedusa (Central Mediterranean) – 1. Influence of transport and identification of different aerosol types</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>G. Pace</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>A. di Sarra</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>D. Meloni</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>S. Piacentino</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>P. Chamard</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">ENEA, Climate Laboratory, Roma, Italy</affiliation>
		<affiliation numeration="2" content_type="html">ENEA, Climate Laboratory, Lampedusa, Italy</affiliation>
	</affiliations>
	<abstract content_type="html">Aerosol optical depth and &amp;#197;ngstr&amp;#246;m exponent were obtained from multi
filter rotating shadowband radiometer (MFRSR) observations carried out at
the island of Lampedusa, in the Central Mediterranean, in the period July
2001&amp;ndash;September 2003. The average aerosol optical depth at 495.7 nm, &amp;tau;,
is 0.24&amp;plusmn;0.14; the average &amp;#197;ngstr&amp;#246;m exponent, &amp;alpha;, is
0.86&amp;plusmn;0.63. The observed values of &amp;tau; range from 0.03 to 1.13, and
the values of &amp;alpha; vary from &amp;minus;0.32 to 2.05, indicating a large
variability in aerosol content and size. In cloud-free conditions, 36% of
the airmasses come from Africa, 25% from Central-Eastern Europe, and
19% from Western France, Spain and the North Atlantic. In summer, 42%
of the airmasses are of African origin. In almost all cases African aerosols
display high values of &amp;tau; and low values of &amp;alpha;, typical of
Saharan dust (average values of &amp;tau; and &amp;alpha; are 0.36 and 0.42,
respectively). Particles originating from Central-Eastern Europe show
relatively large average values of &amp;tau; and &amp;alpha; (0.23 and 1.5,
respectively), while particles from Western France, Spain and the North
Atlantic show the lowest average values of &amp;tau; (0.15), and relatively
small values of &amp;alpha; (0.92). Intermediate values of &amp;alpha; are often
connected with relatively fast changes of the airmass originating sector,
suggesting the contemporary presence of different types of particles in the
air column. The largest values of &amp;alpha; (about 2) were observed in
August 2003, when large scale forest fires in Southern Europe produced
consistent amounts of fine combustion particles that were transported to the
Central Mediterranean by a persistent high pressure system over Central
Europe. Smoke particles in some cases mix with desert dust, producing
intermediate values of &amp;alpha;. The seasonal distribution of the
meteorological patterns over the Mediterranean, the efficiency of the
aerosol production mechanisms, and the variability of the particles&apos;
residence time produce a distinct seasonal cycle of aerosol optical depths
and &amp;#197;ngstr&amp;#246;m exponent values. Particles originating from all sectors
show a summer maximum in aerosol optical depth. The summer increase in
optical depth for European aerosols is linked with an increment in the
values of &amp;alpha; that indicates an enhancement in the number of fine
particles. The summer maximum of &amp;tau; for African particles is associated
with a weak reduction in the &amp;#197;ngstr&amp;#246;m exponent, suggesting an
increase in the total number of particles and a relatively more intense
transport of large particles. The observations were classified according to
the aerosol optical properties, and two main classes have been identified:
desert dust and biomass burning/urban-industrial aerosols. Values of &amp;tau;
and &amp;alpha; averaged over the whole observing period are 0.37 and 0.15 for
desert dust, and 0.27 and 1.77 for urban-industrial/biomass burning
aerosols. Lampedusa reveals a stronger influence of desert dust compared to
other Mediterranean sites (mostly located on the coasts of Europe).</abstract>
	<references>
	</references>
</article>

