Solar neutrino flux, cosmic rays, and the solar activity cycle

Details Solar neutrino flux, cosmic rays, and the solar activity cycle Solar neutrino flux, cosmic rays, and the solar activity cycle

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..104..415r&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 104, April 1986, p. 415-424.

Physics

17

Solar Cosmic Rays, Solar Cycles, Solar Neutrinos, Argon Isotopes, Monte Carlo Method, Particle Production, Statistical Analysis, Sunspot Cycle

Scientific paper

It is suggested that the experimental data on the solar neutrino flux as measured by Davis et al. (1983) from 1970 to 1982 vary with the solar activity cycle to a very high level of statistical significance for all the available tests of the hypothesis (e.g., t-test, run test, Wilcoxon-Mann-Whitney test) when the solar neutrino flux data are computed from the weighted moving averages of order 5. The above tests have also been applied to the data that have been generated by the Monte Carlo simulation with production rate and background rate parameters that are typical of those in the actual experiment. It is shown that the Monte Carlo simulated data do not indicate a variation within the solar cycle. Thus the moving-average data strongly favor the variation within the solar activity cycle.

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