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The conjecture concerning time variations in the solar neutrino fluxThe results of the Fourier transformation of the unequally-spaced time series of the recorded Ar-37 production rate of the solar neutrino experiment (runs 18 to 80, 1970 to 1983) are reviewed. Significance criteria for every period discovered by the harmonic analysis are determined. A Fourier synthesis of certain discovered harmonics are performed. It seems that the solar neutrino flux increases shock-like with a period of approximately 8.3 years and after that breaks down. Possible connections between the periods found by the harmonic analysis and several observed phenomena on the solar surface are indicated.
Document ID
19850026798
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Haubold, H. J. (Academy of Sciences Potsdam (German D.R.)., United States)
Gerth, E. (Academy of Sciences Potsdam (German D.R.)., United States)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 5
Subject Category
Solar Physics
Report/Patent Number
SH-8.1-6
Accession Number
85N35111
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19850026678Collected WorksNineteenth International Cosmic Ray Conference. SH Sessions, Volume 5
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