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The Convection Zone and Oscillations

Published online by Cambridge University Press:  08 February 2017

V.A. Baturin ,
I.V. Mironova  and
S.V. Ayukov
V.A. Baturin
Affiliation:
Sternberg Astronomical Institute, Universitetsky pr., 13, Moscow, Russia
I.V. Mironova
Affiliation:
Sternberg Astronomical Institute, Universitetsky pr., 13, Moscow, Russia
S.V. Ayukov
Affiliation:
Sternberg Astronomical Institute, Universitetsky pr., 13, Moscow, Russia

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We study the influence of the structure and physics of the uppermost superadiabatic layers on the oscillation spectrum of p-modes. These modes are trapped inside the Sun by reflecting at the upper layers of the Sun, so these layers are important for the oscillation spectrum. Indeed, the main difference between the computed and observed frequencies seems to come from these layers (Christensen-Dalsgaard, 1985; Christensen-Dalsgaard and Thompson, 1997).

Type
II. Solar Convection and Variation of Irradiance
Information
Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 85 - 88
Copyright
Copyright © Kluwer 1998 

References

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