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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ACP</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7324</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-8-2797-2008</article-id>
<title-group>
<article-title>Modeling cosmogenic radionuclides &lt;sup&gt;10&lt;/sup&gt;Be and &lt;sup&gt;7&lt;/sup&gt;Be during the Maunder Minimum using the ECHAM5-HAM General Circulation Model</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Heikkilä</surname>
<given-names>U.</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>Beer</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>Feichter</surname>
<given-names>J.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>EAWAG, Dübendorf, Switzerland</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Max-Planck Institute for Meteorology, Hamburg, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>29</day>
<month>05</month>
<year>2008</year>
</pub-date>
<volume>8</volume>
<issue>10</issue>
<fpage>2797</fpage>
<lpage>2809</lpage>
<permissions>
<license xlink:type="simple">
<license-p>This is an open-access article ditributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.</license-p>
</license>
</permissions>
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<abstract>
<p>All existing &lt;sup&gt;10&lt;/sup&gt;Be records from Greenland and Antarctica show increasing
concentrations during the Maunder Minimum period (MM), 1645&amp;ndash;1715, when solar
activity was very low and the climate was colder (little ice age). In detail,
however, the &lt;sup&gt;10&lt;/sup&gt;Be records deviate from each other. We investigate to
what extent climatic changes influence the &lt;sup&gt;10&lt;/sup&gt;Be measured in ice by
modeling this period using the ECHAM5-HAM general circulation model.
Production calculations show that during the MM the mean global &lt;sup&gt;10&lt;/sup&gt;Be
production was higher by 32% than at present due to lower solar activity.
Our modeling shows that the zonally averaged modeled &lt;sup&gt;10&lt;/sup&gt;Be deposition
flux deviates by only ~8% from the average increase of 32%, indicating
that climatic effects are much smaller than the production change. Due to
increased stratospheric production, the &lt;sup&gt;10&lt;/sup&gt;Be content in the downward
fluxes is larger during MM, leading to larger &lt;sup&gt;10&lt;/sup&gt;Be deposition fluxes in
the subtropics, where stratosphere-troposphere exchange (STE) is strongest.
In polar regions the effect is small. In Greenland the deposition change
depends on latitude and altitude. In Antarctica the change is larger in the
east than in the west. We use the &lt;sup&gt;10&lt;/sup&gt;Be/&lt;sup&gt;7&lt;/sup&gt;Be ratio to study changes in
STE. We find larger change between 20&amp;deg; N&amp;ndash;40&amp;deg; N during
spring, pointing to a stronger STE in the Northern Hemisphere during MM. In
the Southern Hemisphere the change is small. These findings indicate that
climate changes do influence the &lt;sup&gt;10&lt;/sup&gt;Be deposition fluxes, but not enough
to significantly disturb the production signal. Climate-induced changes
remain small, especially in polar regions.</p>
</abstract>
<counts><page-count count="13"/></counts>
</article-meta>
</front>
<body/>
<back>
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