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<supportEmail caption="Support">icrc2007@icrc2007.unam.mx</supportEmail>
<title>30th International Cosmic Ray Conference</title>
<description>The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.</description>
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<startDate>2007-07-03T08:00:00</startDate>
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 <title>Long-term Variations in Cosmogenic Be-7 Concentrations with the 11-year Cycle of Solar Activity</title>
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   <name first="Masato" middle="" last="Yoshimori"></name>
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   <title>Prof.</title>
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   <organization>Rikkyo University</organization>
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  <name>Merida, Mexico</name>
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 <abstract>Be-7 radionuclide is (half life 53.3 days) is produced from cosmic ray interactions with atmospheric 
nuclei. We analyzed long-term (1983-2006) variations in surface Be-7 concentrations in Japan 
(geomagnetic latitude ~25N and cutoff rigidity 10 GV) to study an influence of the solar activity. 
The measured Be-7 concentrations in surface air depend on not only a production rate of Be-7 but 
also a transport process in the atmosphere. The measurements indicated that a ratio of Be-7 
concentration in the solar minimum to that in the solar maximum is 1.3-1.4. It is reasonably 
explained from the variations in cosmic ray fluxes between the solar minimum and maximum. We 
concluded that the long-term variations in Be-7 concentrations is mainly caused by the 11-year 
cycle of solar activity and the transport process due to air mass motions does not much contribute 
to the variations in Be-7 concentrations.</abstract>
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