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<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>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys. Discuss.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7375</issn>
<publisher><publisher-name></publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acpd-12-3595-2012</article-id>
<title-group>
<article-title>Effects of cosmic ray decreases on cloud microphysics</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Svensmark</surname>
<given-names>J.</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>Enghoff</surname>
<given-names>M. B.</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>Svensmark</surname>
<given-names>H.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>National Space Institute, Technical University of Denmark, Copenhagen, Denmark</addr-line>
</aff>
<pub-date pub-type="epub">
<day>01</day>
<month>02</month>
<year>2012</year>
</pub-date>
<volume>12</volume>
<issue>2</issue>
<fpage>3595</fpage>
<lpage>3617</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2012 J. Svensmark et al.</copyright-statement>
<copyright-year>2012</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://acp.copernicus.org/preprints/12/3595/2012/acpd-12-3595-2012.html">This article is available from https://acp.copernicus.org/preprints/12/3595/2012/acpd-12-3595-2012.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/preprints/12/3595/2012/acpd-12-3595-2012.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/preprints/12/3595/2012/acpd-12-3595-2012.pdf</self-uri>
<abstract>
<p>Using cloud data from MODIS we investigate the response of cloud microphysics
to sudden decreases in galactic cosmic radiation – Forbush decreases – and
find responses in effective emissivity, cloud fraction, liquid water content,
and optical thickness above the 2–3 sigma level 6–9 days after the minimum in
atmospheric ionization and less significant responses for effective radius
and cloud condensation nuclei (&lt;2 sigma). The magnitude of the signals
agree with derived values, based on simple equations for atmospheric
parameters. Furthermore principal components analysis gives a total
significance of the signal of 3.1 sigma. We also see a correlation between
total solar irradiance and strong Forbush decreases but a clear mechanism
connecting this to cloud properties is lacking. There is no signal in the UV
radiation. The responses of the parameters correlate linearly with the
reduction in the cosmic ray ionization. These results support the suggestion
that ions play a significant role in the life-cycle of clouds.</p>
</abstract>
<counts><page-count count="23"/></counts>
</article-meta>
</front>
<body/>
<back>
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