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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>9</volume_number>
		<issue_number>5</issue_number>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/acpd-9-18235-2009</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/9/18235/2009/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/9/18235/2009/acpd-9-18235-2009.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/9/18235/2009/acpd-9-18235-2009.pdf</fulltext_pdf>
	<start_page>18235</start_page>
	<end_page>18270</end_page>
	<publication_date>2009-09-02</publication_date>
	<article_title content_type="html">Results from the CERN pilot CLOUD experiment</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J. Duplissy</name>
		</author>
		<author numeration="2" affiliations="2">
			<name>M. B. Enghoff</name>
		</author>
		<author numeration="3" affiliations="3">
			<name>K. L. Aplin</name>
		</author>
		<author numeration="4" affiliations="4">
			<name>F. Arnold</name>
		</author>
		<author numeration="5" affiliations="4">
			<name>H. Aufmhoff</name>
		</author>
		<author numeration="6" affiliations="2">
			<name>M. Avngaard</name>
		</author>
		<author numeration="7" affiliations="5">
			<name>U. Baltensperger</name>
		</author>
		<author numeration="8" affiliations="2">
			<name>T. Bondo</name>
		</author>
		<author numeration="9" affiliations="3">
			<name>R. Bingham</name>
		</author>
		<author numeration="10" affiliations="6">
			<name>K. Carslaw</name>
		</author>
		<author numeration="11" affiliations="7">
			<name>J. Curtius</name>
		</author>
		<author numeration="12" affiliations="1">
			<name>A. David</name>
		</author>
		<author numeration="13" affiliations="8">
			<name>B. Fastrup</name>
		</author>
		<author numeration="14" affiliations="9">
			<name>S. Gagné</name>
		</author>
		<author numeration="15" affiliations="1">
			<name>F. Hahn</name>
		</author>
		<author numeration="16" affiliations="10">
			<name>R. G. Harrison</name>
		</author>
		<author numeration="17" affiliations="3">
			<name>B. Kellett</name>
		</author>
		<author numeration="18" affiliations="1">
			<name>J. Kirkby</name>
		</author>
		<author numeration="19" affiliations="9">
			<name>M. Kulmala</name>
		</author>
		<author numeration="20" affiliations="9">
			<name>L. Laakso</name>
		</author>
		<author numeration="21" affiliations="11">
			<name>A. Laaksonen</name>
		</author>
		<author numeration="22" affiliations="12">
			<name>E. Lillestol</name>
		</author>
		<author numeration="23" affiliations="3">
			<name>M. Lockwood</name>
		</author>
		<author numeration="24" affiliations="13">
			<name>J. Mäkelä</name>
		</author>
		<author numeration="25" affiliations="14">
			<name>V. Makhmutov</name>
		</author>
		<author numeration="26" affiliations="2">
			<name>N. D. Marsh</name>
		</author>
		<author numeration="27" affiliations="9">
			<name>T. Nieminen</name>
		</author>
		<author numeration="28" affiliations="1">
			<name>A. Onnela</name>
		</author>
		<author numeration="29" affiliations="8">
			<name>E. Pedersen</name>
		</author>
		<author numeration="30" affiliations="2">
			<name>J. O. P. Pedersen</name>
		</author>
		<author numeration="31" affiliations="2">
			<name>J. Polny</name>
		</author>
		<author numeration="32" affiliations="4">
			<name>U. Reichl</name>
		</author>
		<author numeration="33" affiliations="15">
			<name>J. H. Seinfeld</name>
		</author>
		<author numeration="34" affiliations="9">
			<name>M. Sipilä</name>
		</author>
		<author numeration="35" affiliations="14">
			<name>Y. Stozhkov</name>
		</author>
		<author numeration="36" affiliations="16">
			<name>F. Stratmann</name>
		</author>
		<author numeration="37" affiliations="2">
			<name>H. Svensmark</name>
		</author>
		<author numeration="38" affiliations="2">
			<name>J. Svensmark</name>
		</author>
		<author numeration="39" affiliations="1">
			<name>R. Veenhof</name>
		</author>
		<author numeration="40" affiliations="17">
			<name>Y. Viisanen</name>
		</author>
		<author numeration="41" affiliations="18">
			<name>P. E. Wagner</name>
		</author>
		<author numeration="42" affiliations="5">
			<name>G. Wehrle</name>
		</author>
		<author numeration="43" affiliations="5">
			<name>E. Weingartner</name>
		</author>
		<author numeration="44" affiliations="16">
			<name>H. Wex</name>
		</author>
		<author numeration="45" affiliations="1">
			<name>M. Wilhelmsson</name>
		</author>
		<author numeration="46" affiliations="18">
			<name>P. M. Winkler</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">CERN, Geneva, Switzerland</affiliation>
		<affiliation numeration="2" content_type="html">DTU Space, National Space Institute, Center for Sun-Climate Research, Copenhagen, Denmark</affiliation>
		<affiliation numeration="3" content_type="html">Rutherford Appleton Laboratory, Space Science &amp; Technology Department, Chilton, UK</affiliation>
		<affiliation numeration="4" content_type="html">Max-Planck Institute for Nuclear Physics, Heidelberg, Germany</affiliation>
		<affiliation numeration="5" content_type="html">Paul Scherrer Institut, Laboratory of Atmospheric Chemistry, Villigen, Switzerland</affiliation>
		<affiliation numeration="6" content_type="html">University of Leeds, School of Earth and Environment, Leeds, UK</affiliation>
		<affiliation numeration="7" content_type="html">Goethe-University of Frankfurt, Institute for Atmospheric and Environmental Sciences, Frankfurt am Main, Germany</affiliation>
		<affiliation numeration="8" content_type="html">University of Aarhus, Institute of Physics and Astronomy, Aarhus, Denmark</affiliation>
		<affiliation numeration="9" content_type="html">Helsinki Institute of Physics and University of Helsinki, Department of Physics, Helsinki, Finland</affiliation>
		<affiliation numeration="10" content_type="html">University of Reading, Department of Meteorology, Reading, UK</affiliation>
		<affiliation numeration="11" content_type="html">University of Kuopio, Department of Physics, Kuopio, Finland</affiliation>
		<affiliation numeration="12" content_type="html">University of Bergen, Institute of Physics, Bergen, Norway</affiliation>
		<affiliation numeration="13" content_type="html">Tampere University of Technology, Department of Physics, Tampere, Finland</affiliation>
		<affiliation numeration="14" content_type="html">Lebedev Physical Institute, Solar and Cosmic Ray Research Laboratory, Moscow, Russia</affiliation>
		<affiliation numeration="15" content_type="html">California Institute of Technology, Division of Chemistry and Chemical Engineering, Pasadena, USA</affiliation>
		<affiliation numeration="16" content_type="html">Leibniz Institute for Tropospheric Research, Leipzig, Germany</affiliation>
		<affiliation numeration="17" content_type="html">Finnish Meteorological Institute, Helsinki, Finland</affiliation>
		<affiliation numeration="18" content_type="html">University of Vienna, Institute for Experimental Physics, Vienna, Austria</affiliation>
	</affiliations>
	<abstract content_type="html">During a 4-week run in October–November 2006, a pilot experiment was
performed at the CERN Proton Synchrotron in preparation for the
CLOUD&lt;sup&gt;1&lt;/sup&gt; experiment, whose aim is to study the possible influence of cosmic
rays on clouds. The purpose of the pilot experiment was firstly to carry out
exploratory measurements of the effect of ionising particle radiation on
aerosol formation from trace H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt; vapour and secondly to provide
technical input for the CLOUD design. A total of 44 nucleation bursts were
produced and recorded, with formation rates of particles above the 3 nm
detection threshold of between 0.1 and 100 cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt;s&lt;sup&gt;&amp;minus;1&lt;/sup&gt;, and growth rates between 2
and 37 nm h&lt;sup&gt;&amp;minus;1&lt;/sup&gt;. The corresponding H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt; concentrations were
typically around 10&lt;sup&gt;6&lt;/sup&gt; cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt; or less. The experimentally-measured formation
rates and H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt; concentrations are comparable to those found in the
atmosphere, supporting the idea that sulphuric acid is involved in the
nucleation of atmospheric aerosols. However, sulphuric acid alone is not able
to explain the observed rapid growth rates, which suggests the presence of
additional trace vapours in the aerosol chamber, whose identity is unknown.
By analysing the charged fraction, a few of the aerosol bursts appear to have
a contribution from ion-induced nucleation and ion-ion recombination to form
neutral clusters. Some indications were also found for the accelerator beam
timing and intensity to influence the aerosol particle formation
rate at the highest experimental SO&lt;sub&gt;2&lt;/sub&gt; concentrations of 6 
ppb, although none was found at lower concentrations.
Overall, the exploratory measurements provide suggestive evidence for
ion-induced nucleation or ion-ion recombination as sources of aerosol
particles. However in order to quantify the conditions under which ion
processes become significant, improvements are needed in controlling the
experimental variables and in the reproducibility of the experiments.
Finally, concerning technical aspects, the most important lessons for the
CLOUD design include the stringent requirement of internal cleanliness of the
aerosol chamber, as well as maintenance of extremely stable temperatures
(variations below 0.1&amp;deg;C).
&lt;br&gt;&lt;br&gt;
&lt;sup&gt;1&lt;/sup&gt;CLOUD is an acronym of Cosmics Leaving OUtdoor
Droplets.</abstract>
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