Nonadiabatic effects on the solar p-mode oscillations.

Details Nonadiabatic effects on the solar p-mode oscillations. Nonadiabatic effects on the solar p-mode oscillations.

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997acaps..17..297b&link_type=abstract

Acta Astrophys. Sin., Vol. 17, No. 3, p. 297 - 303

Astronomy and Astrophysics

Astrophysics

Solar Oscillations

Scientific paper

The nonadiabatic frequencies of a standard solar model are discussed. Nonadiabatic effects associated with the radiative losses and convective transfer add small imaginary parts, σi(1) and σi(2), to solar p-mode eigenfrequencies. An asymptotic approximation to the nonadiabatic nonradial p-modes of the Sun is developed. An exact solution of nonadiabatic oscillations, which results in an eigenfrequency equation with a model-dependent surface phase shift, is assumed in the outermost layers, where the asymptotic description is invalid.

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