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SUMMARY:Characteristic Features of the 11-Year Cycle in Cosmic Ray Data*
DTSTART;VALUE=DATE-TIME:20070709T194500Z
DTEND;VALUE=DATE-TIME:20070709T194500Z
DTSTAMP;VALUE=DATE-TIME:20260810T113409Z
UID:indico-contribution-874@cern.ch
DESCRIPTION:Speakers: Dr. LAURENZA\, Monica (INAF/IFSI)\nPast works sugges
 t the existence of several periodicities in comic ray data.\nNevertheless\
 , the reliability of the obtained periods is not often faced.\nIn this pap
 er\, neutron monitor and IMP data were analysed by using the Fast\nFourier
  Transform and Wavelet techniques to determine the reliability of each\nid
 entified medium- and long-term periodicity. Moreover\, their relevance is\
 nanalysed along the solar cycle evolution to better understand their role 
 in\nthe 11-year cosmic ray cycle.\n\n*: Work supported by the Italian Spac
 e Agency for BepiColombo Mission.\n\nhttps://indico.nucleares.unam.mx/even
 t/4/session/40/contribution/874
LOCATION:Merida\, Mexico Regency (Hyatt)
URL:https://indico.nucleares.unam.mx/event/4/session/40/contribution/874
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