Helioseismology, Neutrinos and Radiative Zones

@article{Turckchize2005HelioseismologyNA,
  title={Helioseismology, Neutrinos and Radiative Zones},
  author={S. Turck-chi{\`e}ze and S. CouvidatL. Piau},
  journal={Eas Publications Series},
  year={2005},
  volume={17},
  pages={149-154}
}
The solar interior has been scrutinized by two different and independent probes during the last twenty years with important revi- sions of the solar model, including a recent heavy element abundance revision. Today, we get a quantitatively coherent picture (even incom- plete) of the solar (stellar) radiative zones. In this review, we recall the clues for solar gravitational settling definitively established by the seis- mic determination of the photospheric helium content. We comment also on… 

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References

SHOWING 1-3 OF 3 REFERENCES
Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis in honor of David L. Lambert
We review our current knowledge of the solar chemical composition as determined from photospheric absorption lines. In particular we describe the recent significant revisions of the solar abundances
Origin and evolution of the elements
This work on the origin and evolution of cosmic elements draws upon the work of experts at an international conference held in Paris in 1992. It deals with stellar and primordial nuceosynthesis,