The fundamental mode of nonradial, nonadiabatic stellar oscillation

Details The fundamental mode of nonradial, nonadiabatic stellar oscillation The fundamental mode of nonradial, nonadiabatic stellar oscillation

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..562z&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Sept. 1982, p. 562-565) Soviet Astronomy Letters (ISSN 0360-0327), vol. 8, Sept.-Oct

Astronomy and Astrophysics

Astronomy

1

Nonadiabatic Conditions, Stellar Oscillations, Adiabatic Conditions, Convection, Solar Oscillations, Vibration Mode

Scientific paper

Fundamental-mode nonadiabatic oscillations of a star that have a large value for the order l of the spherical harmonic are examined. Oscillations of this type have been observed on the sun as one branch of the two-dimensional spectrum for the 5-min oscillations. A system of energy equations for nonadiabatic oscillations is derived and applied to the fundamental mode of high-1, nonradial, nonadiabatic oscillation. It is shown that the f-mode of the 5-min oscillation on the sun can be excited only through interaction with a turbulent convection.

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