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  <organization>ICN-UNAM</organization>
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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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<closed>True</closed>
<location>
 <name>Merida, Mexico</name>
 <address></address>
 <room></room>
</location>
<startDate>2007-07-03T08:00:00</startDate>
<endDate>2007-07-11T19:00:00</endDate>
<creationDate>2005-09-26T05:04:53</creationDate>
<modificationDate>2024-04-12T17:46:55</modificationDate>
<timezone>Mexico/General</timezone>
<chair>
 <user>
  <title>Dr.</title>
  <name first="José" middle="" last="Valdés"></name>
  <organization>IGeof-UNAM</organization>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
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 <board>201 (10B)</board>
 <track>SH.3.2</track>
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 <title>The 120-yrs solar cycle of the cosmogenic isotopes</title>
 <speakers>
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   <title>Dr.</title>
   <name first="Victor Manuel" middle="" last="Velasco Herrera"></name>
   <organization>Universidad Nacional Autonoma de Mexico, Instituto de Geofisica</organization>
   <emailHash>e850c8550923689365acf95418ce657e</emailHash>
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   <title>Dr.</title>
   <name first="Victor Manuel" middle="" last="Velasco Herrera"></name>
   <organization>Universidad Nacional Autonoma de Mexico, Instituto de Geofisica</organization>
   <emailHash>e850c8550923689365acf95418ce657e</emailHash>
  </user>
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   <title>Dr.</title>
   <name first="José" middle="" last="Valdés-Galicia"></name>
   <organization>Universidad Nacional Autonoma de Mexico, Instituto de Geofisica</organization>
   <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Blanca" middle="" last="Mendoza"></name>
   <organization>Universidad Nacional Autonoma de Mexico, Instituto de Geofisica</organization>
   <emailHash>9bdab64740f6219c1663c2f525a4a7ef</emailHash>
  </user>
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 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Regency (Hyatt)</room>
 </location>
 <startDate>2007-07-09T14:45:00</startDate>
 <endDate>2007-07-09T14:45:00</endDate>
 <abstract>The solar periodicities of 80-88 yrs (Gleissberg cycle) and 205 yrs (de Vries cycle or Suess cycle) using different 
time series of proxies of cosmogenic isotopes have been reported in a great number of papers.
In this work we present a more objective and general cycle-length determination applying the wavelet 
transformation based on the Morlet wavelet to the cosmogenic isotopes. We use the INTERCAL98 for C14 time 
series and Be10 time series for both the South and North Poles. The results obtained from the wavelet 
transformation show that there are no periodicities of 80-88 yrs or 205 yrs. This suggests that these periodicities 
may be the result of applying transformations to time series that do not fulfill the condition of stationary.

The estimated periodicities obtained the from Morlet wavelet are of 60 yrs (Yoshimura-Gleissberg cycle), 120 yrs 
and 240 yrs (de Vries cycle or Suess Cycle). The 120-periodicity could possibly be one of the principal periodicities 
of magnetic solar activity.</abstract>
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