Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-07-30
Astrophysical Journal 540 (2000) 1109; Erratum 544 (2000) 1181
Astronomy and Astrophysics
Astrophysics
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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