Solar Heavy-Element Abundance: Constraints from Frequency Separation Ratios of Low-Degree p-Modes

@article{Chaplin2007SolarHA,
  title={Solar Heavy-Element Abundance: Constraints from Frequency Separation Ratios of Low-Degree p-Modes},
  author={William J. Chaplin and Aldo M. Serenelli and Sarbani Basu and Yvonne P. Elsworth and Roger New and Graham A. Verner},
  journal={The Astrophysical Journal},
  year={2007},
  volume={670},
  pages={872-884}
}
We use very precise frequencies of low-degree solar-oscillation modes measured from 4752 days of data collected by the Birmingham Solar-Oscillations Network to derive seismic information on the solar core. We compare these observations to results from a large Monte Carlo simulation of standard solar models, and use the results to constrain the mean molecular weight of the solar core and the metallicity of the solar convection zone. We find that only a high value of solar metallicity is… Expand
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