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Cosmic ray secular variations in terrestrial records and auroraeThe rediscovery that the Sun and the solar wind can undergo important changes on historical time scales has brought into question the stability of the cyclic behavior of past time series of solar and solar-terrestrial origin. It was found by Vector Fourier analysis that the solar 11 year cycle is present in the series of 10Be, delta 180, in ice cores and of thermoluminescence (TL) in sea sediments during the last Millennia with a frequency modulation, related to the Sun behavior, as tested by comparison with the Sunspot number R sub z series. It was shown that the cyclogram of the series of yearly Aurorae from 1721 to 1979 linear-regression-corrected-for-R sub z is straight for the periodicity zeta=11,1y, which indicates that such periodicity is constant in time corresponding to the only line present in the 11y band. The maxima of this component appear at the same time together with the high speed solar wind streams taking place in coronal holes situated in high heliolatitudes. It is evidenced that the 11 year cycle has undergone frequency oscillations on a time scale of two centuries, although it is very difficult to determine the periodicities with high accuracy.
Document ID
19850026783
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Attolini, M. R.
(Consiglio Nazionale delle Ricerche Turin, Italy)
Castagnoli, G. C.
(Torino Univ. Turin, Italy)
Bonino, G.
(Torino Univ.)
Galli, M.
(Bologna Univ.)
Nanni, T.
(Consiglio Nazionale delle Ricerche)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 5
Subject Category
Space Radiation
Report/Patent Number
SH-7.1-3
Accession Number
85N35096
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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