Searching for Deep Changes of the Solar Structure

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

A relation between normal-mode and multiple-reflection time-distance data is derived by applying the principle of stationary phase to solar acoustic oscillations. This relation links the global and local helioseismology data, and provides estimates of acoustic travel times in terms of mode frequencies. It is employed for searching solar-cycle variations in the tachocline, by using GONG and MDI data of 1996-2002. The time-distance signature of magnetic field at the base of the convection zone recently reported by Chou and Serebryanskiy (2002) and the current precision of the deep changes are discussed.

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