Spacetime Modulation of Solar Neutrino Flux: 1970--1992

Astronomy and Astrophysics – Astronomy

Scientific paper

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Elementary Particles, Sun: Activity, Sun: Magnetic Fields, Sun: Particle Emission

Scientific paper

Clues for a north-south asymmetry in the solar neutrino flux, as measured by the Homestake experiment, were found over the period 1970-1992. This asymmetry seems to play an important role in the frame of a possible solar neutrino modulation related to solar activity features. We have employed the green corona line data (GCL; spectral line Fe XIV 530.3 mm), both for the total intensity and divided into heliographic latitudinal belts, as tracers of the solar magnetic fields. Our findings confirm the recent work of Oakley et al., supporting the idea that the Homestake data modulation originated from the neutrino interaction with the solar magnetic field in the equatorial zone. Moreover, we show that the correlation increases by a factor of about 1.75 when only the southern neutrino flux is correlated with the brightness of the equatorial GCL.

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