Solar neutrino: Flux, cosmic rays and the 11 year solar cycle

Details Solar neutrino: Flux, cosmic rays and the 11 year solar cycle Solar neutrino: Flux, cosmic rays and the 11 year solar cycle

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..438r&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 438-441 (SEE N85-34991 23-93)

Physics

Rays, Solar Cycles, Solar Flux, Solar Neutrinos, Sun, Sunspots, Maximum Likelihood Estimates, Monte Carlo Method, Rates (Per Time), Simulation

Scientific paper

It is shown that the results of maximum likelihood treatment of Monte Carlo simulation with constant production rate of 7.6 SNU and 1.Epsilon SNU are consistent with the constant production rate when the tests of hypotheses (e.g., t-test, sigma squared-test, Wilcoxon-Mann-Whitney test, run test, etc.) are applied to the two groups of data formed from sunspot minimum range and sunspot maximum range, whereas the real data pulsates with the solar activity cycle. It is shown that SN flux-change is in opposition phase to the solar activity cycle and lags behind the latter by about one year. A correlation between SN flux and the cosmic rays is suggested.

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