Author:
Baturin V.A.,Mironova I.V.,Ayukov S.V.
Abstract
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).
Publisher
Cambridge University Press (CUP)