Asymptotic method for solving an inverse problem of solar seismology

Details Asymptotic method for solving an inverse problem of solar seismology Asymptotic method for solving an inverse problem of solar seismology

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..438b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, May 1987, p. 438-443. In Russian. In Russian.

Statistics

Computation

8

Asymptotic Methods, Computational Astrophysics, Helioseismology, Solar Activity, Acoustic Velocity, Differential Equations, Phase Shift, Solar Interior

Scientific paper

A technique for the solution of the inverse problem for the solar 5-minute oscillations is proposed. This technique provides an independent determination of the sound speed as a function of depth in the solar interior and the frequency dependence of the effective phase shift for the reflection of the trapped acoustic waves from the outer layers. The preliminary numerical results are presented.

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