Solar neutrinos and nonradial oscillations of the sun

Details Solar neutrinos and nonradial oscillations of the sun Solar neutrinos and nonradial oscillations of the sun

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980dossr.251r1342z&link_type=abstract

(Akademiia Nauk SSSR, Doklady, vol. 251, no. 6, 1980, p. 1342-1345.) Soviet Physics - Doklady, vol. 25, Apr. 1980, p. 219-221. T

Physics

Gravity Waves, Solar Neutrinos, Solar Oscillations, Solar Physics, Periodic Variations, Vibration Mode, Wave Attenuation, Wave Propagation

Scientific paper

It is shown that surface oscillations of the sun with a period of 2 hours, 40 minutes are a weak echo of intense adiabatic oscillations of the solar interior, wherein the lower quadrupole g-mode is excited by thermonuclear energy sources. For the quadrupole g-mode to have a period of 2 hours, 40 minutes and to become sharply attenuated in the solar mantle, it is sufficient for the outer part of the interior to be close convective equilibrium. This quasi-equilibrium of the solar interior may explain the low counting rate of solar neutrinos in chlorine detectors.

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