Computer Science – Sound
Scientific paper
Dec 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..539k&link_type=abstract
In ESA, Seismology of the Sun and Sun-Like Stars p 539-543 (SEE N89-25819 19-92)
Computer Science
Sound
2
Acoustic Velocity, Solar Spectra, Sound Waves, Velocity Distribution, Acoustic Frequencies, Asymmetry, Spectrum Analysis, Stellar Models
Scientific paper
The effect on the solar acoustic frequency spectrum of a localized deviation from spherical symmetry concentrated near the outer convective zone of the Sun is studied. The local asymmetry is modelled by an angular-dependent contribution to the sound speed. Acoustic frequencies in the range 1500 to 4000 microHz were calculated for a nonspherical deformation of relative amplitude epsilon varying from 0 to 0.1. For epsilon less than 0.02 all acoustic frequencies of this range are strongly and irregularly displaced (quantum chaos). For lower values only a small fraction of the frequencies are irregularly shifted. The deviation of the frequency spectrum of the deformed solar model with respect to the spectrum of a spherically symmetric model is measured by a relative scatter. The relative scatter of the observed solar frequencies with respect to the frequencies of a standard spherically symmetric solar model is found to correspond to an amplitude of the disturbance epsilon = 0.025. Results indicate that even slight local asymmetries influence the precise positions of the frequencies. They suggest the possibility of a diagnosis of nonspherical effects in the structure of the Sun.
Kosovichev Aleksandr G.
Perdang J.
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