Time variations of the solar neutrino flux

Details Time variations of the solar neutrino flux Time variations of the solar neutrino flux

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.112..397h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 112, no. 2, May 1985, p. 397-405.

Astronomy and Astrophysics

Astrophysics

7

Argon Isotopes, Fourier Analysis, Solar Neutrinos, Harmonic Analysis, Power Spectra, Secular Variations, Solar Flux Density

Scientific paper

The Fourier analysis of the argon-37 production rate for runs 18 - 80 observed in Davis's well-known solar neutrino experiment is presented. The method of Fourier analysis with the unequally-spaced data of Davis and associates is described and the discovered periods are compared with recently published results for the analysis of the data of runs 18 - 69. The harmonic analysis of the data of runs 18 - 80 shows time variations of the solar neutrino flux with periods π = 8.33, 5.26, 2.13, 1.56, 0.83, 0.64, 0.54, and 0.50 yr, respectively, which confirms earlier computations.

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