A Possible Correlative Time Variation in the Production Rates of the Neutrinos from the p-p Reactions and the Boron-8 Decay Processes in the Solar Core

Details A Possible Correlative Time Variation in the Production Rates of the Neutrinos from the p-p Reactions and the Boron-8 Decay Processes in the Solar Core A Possible Correlative Time Variation in the Production Rates of the Neutrinos from the p-p Reactions and the Boron-8 Decay Processes in the Solar Core

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....3.1247s&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

Both of the observational results from the Homestake and the Gallex, now GNO experiments have been made in use to find some possible time variation in the neutrino fluxes from the p-p reactions and the Boron-8 decay processes. It is suggested out that the production rates of the neutrinos from these two processes have a tendency to vary quasi-biennially. Since it seems that this tendency is further correlated with the distribution of the magnetic fields inside the convective layer of the sun, the emission of the neutrinos generated from the proton-proton chain reactions in the solar core may be modified by the growth and decay of these magnetic fields.

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