Physics
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..128....3g&link_type=abstract
(IAU, The Inside the Sun Colloquium, 121st, Versailles, France, May 22-26, 1989) Solar Physics (ISSN 0038-0938), vol. 128, July
Physics
9
Solar Flares, Solar Interior, Solar Magnetic Field, Convection Cells, Electric Fields, Nuclear Fusion, Particle Beams, Solar Neutrinos
Scientific paper
It is assumed that at the solar core finite amplitude flows are generated by some process for which a candidate can be the planetary tides. It is also assumed that there are some local magnetic flux bundles at the solar core with a strength larger than 1000 G. The aim of this paper is to show that these assumptions involve an electric field generation which then produces local thermonuclear runaways which shoot up convective cells to the outer layers. Within certain conditions, these primal convective cells erupt in the subphotospheric layers, which phenomenon can produce high-energy particle beams which when injected into magnetic flux tubes appear as flares. These processes are suggested for solving the neutrino problem, and also to interpret the spiky character of the solar neutrino flux and the correlation of the energy production of the sun with its atmospheric activity.
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