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<!DOCTYPE article SYSTEM "http://www.atmos-chem-phys.net/inc/acp/copernicus.dtd">
<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>4</volume_number>
		<issue_number>7</issue_number>
		<publication_year>2004</publication_year>
	</journal>
	<doi>10.5194/acp-4-2015-2004</doi>
	<article_url>http://www.atmos-chem-phys.net/4/2015/2004/</article_url>
	<abstract_html>http://www.atmos-chem-phys.net/4/2015/2004/acp-4-2015-2004.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys.net/4/2015/2004/acp-4-2015-2004.pdf</fulltext_pdf>
	<start_page>2015</start_page>
	<end_page>2023</end_page>
	<publication_date>2004-10-05</publication_date>
	<article_title content_type="html">Atmospheric particle formation events at Värriö measurement station in Finnish Lapland 1998-2002</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>H. Vehkamäki</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>M. Dal Maso</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>T. Hussein</name>
		</author>
		<author numeration="4" affiliations="1,4">
			<name>R. Flanagan</name>
		</author>
		<author numeration="5" affiliations="2">
			<name>A. Hyvärinen</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>J. Lauros</name>
		</author>
		<author numeration="7" affiliations="1">
			<name>P. Merikanto</name>
		</author>
		<author numeration="8" affiliations="1">
			<name>M. Mönkkönen</name>
		</author>
		<author numeration="9" affiliations="1">
			<name>K. Pihlatie</name>
		</author>
		<author numeration="10" affiliations="2">
			<name>K. Salminen</name>
		</author>
		<author numeration="11" affiliations="1">
			<name>L. Sogacheva</name>
		</author>
		<author numeration="12" affiliations="2">
			<name>T. Thum</name>
		</author>
		<author numeration="13" affiliations="1">
			<name>T. M. Ruuskanen</name>
		</author>
		<author numeration="14" affiliations="1">
			<name>P. Keronen</name>
		</author>
		<author numeration="15" affiliations="1">
			<name>P. P. Aalto</name>
		</author>
		<author numeration="16" affiliations="3">
			<name>P. Hari</name>
		</author>
		<author numeration="17" affiliations="1">
			<name>K. E. J. Lehtinen</name>
		</author>
		<author numeration="18" affiliations="1">
			<name>Ü Rannik</name>
		</author>
		<author numeration="19" affiliations="1">
			<name>M. Kulmala</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Department of Physical Sciences, P.O. Box 64, 00014 University of Helsinki, Finland</affiliation>
		<affiliation numeration="2" content_type="html">Finnish Meteorological Institute, P.O Box 503, 00101 Helsinki, Finland</affiliation>
		<affiliation numeration="3" content_type="html">Department of Forest Ecology, P.O. Box 27, 00014 University of Helsinki, Finland</affiliation>
		<affiliation numeration="4" content_type="html">Dep. of Experimental Physics and Environmental Change Institute, National Univ. of Ireland, Galway, University Road Galway, Ireland</affiliation>
	</affiliations>
	<abstract content_type="html">During the calendar years 1998-2002, 147 clear 8nm diameter particle
formation events have been identified at the SMEAR I station in
V&amp;#228;rri&amp;#246;, northern Finland. The events have been classified in detail
according to the particle formation rate, growth rate, event starting time,
different trace gas concentrations and pre-existing particle concentrations
as well as various meteorological conditions. The frequency of particle
formation and growth events was highest during the spring months between
March and May, suggesting that increasing biological activity might produce
the precursor gases for particle formation. The apparent 8nm particle
formation rates were around 0.1 /cm&lt;sup&gt;3&lt;/sup&gt;s, and they were uncorrelated with
growth rates that varied between 0.5 and 10nm/h. The air masses with
clearly elevated sulphur dioxide concentrations (above 1.6ppb) came, as
expected, from the direction of the Nikel and Monschegorsk smelters. Only 15
formation events can be explained by the pollution plume from these sources.</abstract>
	<references>
	</references>
</article>

