On the p-mode spectrum of solar models

Details On the p-mode spectrum of solar models On the p-mode spectrum of solar models

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...281..551g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 281, no. 2, p. 551-560

Astronomy and Astrophysics

Astrophysics

14

Helioseismology, P Waves, Solar Oscillations, Solar Spectra, Stellar Evolution, Stellar Models, Boundary Conditions, Equations Of State, Gravitational Effects, Mathematical Models, Solar Gravitation, Stellar Composition

Scientific paper

We report seismological results of a new improved standard solar model
which for low and intermediate degrees reproduces the observations
within a few micro-Hz. The influence of the gravitational contraction,
of the solar age, of the equation of state, of a varying mixing length
and of the surface boundary condition is also considered.

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