Short-time variations of the solar neutrino luminosity

Details Short-time variations of the solar neutrino luminosity Short-time variations of the solar neutrino luminosity

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...10..389h&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 10 (A85-22801

Physics

Annual Variations, Luminosity, Solar Neutrinos, Gravity Waves, Solar Flux Density, Solar Oscillations

Scientific paper

The solar neutrino observations of Davis et al. (1982) are used to search for short-time variations of the solar neutrino luminosity. The Fourier transform of the Davis data shows that the Ar-37 production rate pulses with multiple periods in the order of years. The results confirm those of Sakurai (1979), who showed that there is evidence that the observed solar neutrino flux has a tendency to vary with quasi-biennial periodicity.

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