The conjecture concerning time variations in the solar neutrino flux

Details The conjecture concerning time variations in the solar neutrino flux The conjecture concerning time variations in the solar neutrino flux

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..434h&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 434-437 (SEE N85-34991 23-93)

Physics

Argon Isotopes, Fourier Transformation, Harmonic Analysis, Solar Flux, Solar Neutrinos, Sun, Time Series Analysis, Harmonics, Stochastic Processes

Scientific paper

The 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.

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