Attempts to infer the density distribution in the outer part of the Sun from p-mode oscillations spectrum

Solar Physics - Tập 133 - Trang 117-125 - 1991
Hiromoto Shibahashi1
1Department of Astronomy, Faculty of Science, University of Tokyo, Tokyo, Japan

Tóm tắt

We devise two asymptotic inversion methods of inferring the density distribution in the outer part of the Sun from the p-mode frequency spectrum of the Sun. One of them is based on an integral equation of nonlinear inversion, while the other reduces the problem to a linear form which is derived from comparison of the observed eigenfrequencies of the true Sun and the theoretical eigenfrequencies of a solar model.

Tài liệu tham khảo

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