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scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

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STP12 Abstracts<br />

Berlin, 12 - 16 July <strong>2010</strong><br />

SCOSTEP Symposium <strong>2010</strong><br />

Variability of solar activity <strong>an</strong>d cosmic rays, <strong>an</strong>d their influences on climate ch<strong>an</strong>ge<br />

Miyahara Hiroko 1 , Yokoyama Yusuke 1 , Yamaguchi Yasuhiko 1 , Nakatsuka Takeshi 2 , Horiuchi Kazuho<br />

3 , Fallon Stewart 4 , Matsuzaki Hiroyuki 1<br />

1 2 3 4<br />

The University of Tokyo, Nagoya University, Hirosaki University, The Australi<strong>an</strong> National<br />

University<br />

In this paper, we discuss the long-term variation of solar activity during the last 6000<br />

years, based on the frequency <strong>an</strong>alyses of <strong>an</strong>nually measured carbon-14 content in tree rings.<br />

The long-term variations of solar activity are often reconstructed based on decadal data of<br />

cosmogenit nuclides, however, it is difficult to eliminate the variations caused by the ch<strong>an</strong>ges<br />

in climate ch<strong>an</strong>ge, <strong>an</strong>thropogenic effect <strong>an</strong>d the geomagnetic field intensity. So far, multiple<br />

scenarios for the long-term variation of solar activity level have been <strong>der</strong>ived based on<br />

the data sets of cosmogenit nuclides. Our previous studies have shown that the actual length<br />

of solar decadal cycle may be <strong>an</strong>other independent reference for the absolute level of solar<br />

activity. Our records obtained so far indicate that the lengths have varied within 8-15 years<br />

depending on the level of long-term solar activity.<br />

In this paper, we also discuss the variability of the flux of galactic cosmic rays at the earth<br />

related to the variation of solar magnetic activity since the Early Medieval Maximum Period.<br />

We apply the records of multiple cosmogenic nuclides with <strong>an</strong>nual resolution to <strong>der</strong>ive the<br />

information on the variation of incident cosmic rays in the past. The reconstructed variation of<br />

cosmic rays shows that the components of the 11-year <strong>an</strong>d 22-year variations in cosmic rays<br />

vary in time depending on the long-term level of solar magnetic activity. These characteristic<br />

variations of cosmic rays have been also detected in the reconstructed northern hemispheric<br />

temperatures <strong>an</strong>d the humidity ch<strong>an</strong>ge in Jap<strong>an</strong>, <strong>an</strong>d thus it is suggested that cosmic rays are<br />

playing import<strong>an</strong>t role in climate ch<strong>an</strong>ge at the hemispheric scale.

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