Can variations of sunspot number be related to those of the solar neutrino flux?

Details Can variations of sunspot number be related to those of the solar neutrino flux? Can variations of sunspot number be related to those of the solar neutrino flux?

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..131..407v&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 131, Feb. 1991, p. 407-410.

Physics

Neutrino Beams, Solar Flares, Solar Interior, Solar Neutrinos, Sunspots, Charged Particles, Energetic Particles, Particle Interactions, Wave Interaction

Scientific paper

A hypothesis that nondissipating wave-bound beam structures may be created in plasma due to interaction between energetic charged particles and undamped Van Kampen (1955) waves. This hypothesis, if correct, might account for several phenomena observed in the sun. For instance, on entering the atmosphere and then decaying, the structures may lead to flares. Furthermore, the idea offers propitious prospects of solving the well-known problem of the solar neutrino deficit. In addition, a relation between phenomena occurring within the sun's core and those on its surface becomes possible.

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