Physics
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ssrv...38..243s&link_type=abstract
Space Science Reviews (ISSN 0038-6308), vol. 38, July-Aug. 1984, p. 243-279.
Physics
4
Solar Cycles, Solar Flux Density, Solar Neutrinos, Solar Terrestrial Interactions, Stellar Cores, Variable Stars, Climatology, Dendrochronology, Radioactive Age Determination, Secular Variations, Solar Activity, Solar Physics, Thermonuclear Reactions
Scientific paper
Neutrino flux observational data are the basis of the present consideration of physical (thermonuclear) processes in the solar core. Both the efficiency of the outward transport of the nuclear energy released in the core, and the location of the lower boundary of the convective layer inside the sun, may be sufficiently variable, periodically, to produce the observed, quasi-biennial periodicity in the neutrino flux from the sun. The origin of solar activity and luminosity variabilities on the scale of about 100 years may lie in a causal relation to a mechanism that is triggered by a rearrangement of the sun's internal structure. This rearrangement may be forced by efficiency variations in the solar core's thermonuclear reactions, and could be responsible for the variability of the luminosity and the activity of the sun
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