Simple Seismic Tests of the Solar Core

Astronomy and Astrophysics – Astrophysics

Scientific paper

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8 pages, 4 figures, uses AASTeX; revised for publication; accepted by Astrophysical Journal

Scientific paper

10.1086/309388

A model-independent reconstruction of mechanical profiles (density, pressure)
of the solar interior is outlined using the adiabatic sound speed and bouyancy
frequency profiles. These can be inferred from helioseismology if both p- and
g-mode frequencies are measured. A simulated reconstruction is presented using
a solar model bouyancy frequency and available sound speed data.

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