Dec 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mmsai..51..611c&link_type=abstract
(Società Astronomica Italiana, Convegno sulla Variabilita Stellare, 1st, Massalubrense, Italy, May 22-24, 1980.) Società Astrono
Physics
Convection, Solar Oscillations, Solar Physics, Abundance, Diameters, Radial Velocity
Scientific paper
Theoretical and observational problems in the study of solar oscillations are reviewed. Consideration is given to models of solar pulsations, for which accurate values of initial solar abundances and a more complete knowledge of convective zone dynamics are required. Measurements of variations in the solar diameter or the radial velocity of the center of the solar disk are then discussed, and arguments are presented in favor of the terrestrial origin of the 160-min solar oscillations. The importance of the study of short-period (about 5 min) solar oscillations to theories of the solar convective zone is also pointed out.
Cavallini Fabio
Ceppatelli Guido
Righini Alberto
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