Physics
Scientific paper
Sep 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981zhpmr..34..289k&link_type=abstract
(ZHETF Pis'ma v Redaktsiiu, vol. 34, Sept. 5, 1981, p. 289-292.) JETP Letters, vol. 34, Sept. 5, 1981, p. 275-278. Translation.
Physics
Seismic Waves, Solar Activity, Solar Cycles, Solar Gravitation, Solar Neutrinos, Solar Oscillations, Adiabatic Conditions, Cores, Particle Flux Density, Solar Cosmic Rays, Solar Physics, Stellar Models
Scientific paper
The paper examines the possible excitation of gravitational oscillations of the solar core which may be responsible for a 2-yr cycle in the flux of solar neutrinos. It is shown that a natural mechanism for the modulation may be the excitation of a low-lying gravitational mode, assuming that the solar core is near an adiabatic equilibrium. The possibility of a 11-yr variation in the flux is discussed, which must have an index lower than that of the 2-yr modulation.
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