Simple Seismic Tests of the Solar Core
Astrophysics
2009-10-31 v7
Abstract
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.
Keywords
Cite
@article{arxiv.astro-ph/9907447,
title = {Simple Seismic Tests of the Solar Core},
author = {Dallas C. Kennedy},
journal= {arXiv preprint arXiv:astro-ph/9907447},
year = {2009}
}
Comments
8 pages, 4 figures, uses AASTeX; revised for publication; accepted by Astrophysical Journal