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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>8</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2008</publication_year>
	</journal>
	<doi>10.5194/acpd-8-13265-2008</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/8/13265/2008/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/8/13265/2008/acpd-8-13265-2008.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/8/13265/2008/acpd-8-13265-2008.pdf</fulltext_pdf>
	<start_page>13265</start_page>
	<end_page>13299</end_page>
	<publication_date>2008-07-14</publication_date>
	<article_title content_type="html">Cosmic rays, CCN and clouds – a reassessment using MODIS data</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J. E. Kristjánsson</name>
			<email>j.e.kristjansson@geo.uio.no</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>C. W. Stjern</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>F. Stordal</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>A. M. Fjǽraa</name>
		</author>
		<author numeration="5" affiliations="3">
			<name>G. Myhre</name>
		</author>
		<author numeration="6" affiliations="4">
			<name>K. Jónasson</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Department of Geosciences, University of Oslo, Oslo, Norway</affiliation>
		<affiliation numeration="2" content_type="html">Norwegian Institute for Air Research, Kjeller, Norway</affiliation>
		<affiliation numeration="3" content_type="html">Center for International Climate and Environmental Research, Oslo, Norway</affiliation>
		<affiliation numeration="4" content_type="html">Department of Mathematics, University of Iceland, Reykjavík, Iceland</affiliation>
	</affiliations>
	<abstract content_type="html">The response of clouds to sudden decreases in the flux of galactic cosmic
rays (Forbush decrease events) has been investigated using cloud products
from the space-borne MODIS instrument, which has been in operation since
2000. By focusing on pristine Southern Hemisphere ocean regions we examine
areas which are particularly susceptible to changes in cloud condensation
nuclei (CCN) concentrations, and where a cosmic ray signal should be easier
to detect than elsewhere. While previous studies on the subject have mainly
considered cloud cover, the high spatial and spectral resolution of MODIS
allows for a more thorough study of microphysical parameters such as cloud
droplet size, cloud water content and cloud optical depth, in addition to
cloud cover. Averaging the results from the 13 Forbush decrease events that
were considered, no systematic correlation was found between any of the four
cloud parameters and galactic cosmic radiation, with a seemingly random
distribution of positive and negative correlations. When only the three
Forbush decrease events with the largest amplitude are studied, the
correlations fit the hypothesis better, with 8 out of 12 correlations having
the expected sign. Splitting the area of study into several sub-regions, one
sub-region in the Atlantic Ocean showed statistically significant
correlations compatible with a cosmic ray-induced enhancement of CCN and
cloud droplet number concentrations. However, the lack of correlation in any
of the other 5 sub-regions suggests that this may be a statistical
co-incidence. Introducing a time lag of a few days for clouds to respond to
the cosmic ray signal did not change the overall results. Singling out low
clouds of intermediate optical depth with large susceptibility did not lead
to higher correlations. In conclusion, no response to variations in cosmic
rays associated with Forbush decrease events was found in marine low clouds
in remote regions using MODIS data.</abstract>
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