A possible mechanism to cause the quasi-biennial variability on the solar neutrino flux

Details A possible mechanism to cause the quasi-biennial variability on the solar neutrino flux A possible mechanism to cause the quasi-biennial variability on the solar neutrino flux

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..430s&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 430-433 (SEE N85-34991 23-93)

Physics

Annual Variations, Solar Flux, Solar Neutrinos, Stellar Structure, Sun, Nonlinearity, Simulation, Solar Interior, Solar Temperature

Scientific paper

It is suggested that the quasi-biennial change in the observed flux of the solar neutrinos is causally related to some non-linear process at the central core of the Sun, being associated with the charge in the central temperature. This process seems to be responsible for the physical adjustment of the internal structure of the Sun. Numerical simulation on this process is able to reproduce the quasi-biennial change in the flux of these neutrinos.

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