Advertisement

About solar model calibration

  • P. Morel
  • G. Berthomieu
  • J. Provost
  • Y. Lebreton
Contributed Papers
Part of the Lecture Notes in Physics book series (LNP, volume 458)

Abstract

A new value of the ratio of the heavy elements content to hydrogen abundance Z/X has been recently estimated in the solar atmosphere. We present the consequences of this result on the solar standard model and we examine the sensitivity to Z/X of the solar neutrinos flux predictions and of the oscillation frequencies.

Keywords

Convection Zone Solar Model Iron Abundance Solar Standard Model Hydrogen Abundance 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. Anguera Gubau M., Palle P., Perez Hernandez F., Regulo C. Roca Cortes T. 1992, Astron. Astrophys., 255, 363–372ADSGoogle Scholar
  2. Berthomieu. G., Provost. J., Morel. P., Lebreton. Y., 1993, Astron. Astrophys., 268, 775–791ADSGoogle Scholar
  3. Christensen-Dalsgaard J., 1991, in Challenges to Theories of the Structure of Moderate-Mass Stars, D.O. Gough, J. Toomre (Eds), Springer Verlag, p 11–36Google Scholar
  4. Christensen-Dalsgaard J., Gough D.O., Morgan J.G., 1979, Astron. Astrophys., 73, 121–128ADSGoogle Scholar
  5. Grevesse, N., 1991, in Evolution of Stars: The Photospheric Abundance Connection, Eds. Michaud G., Tutukov A., IAU, 63Google Scholar
  6. Grevesse N., Noels A., Sauval A.J., 1992, Proceedings of the first SOHO Workshop, Annapolis ESA SP-348, p 305Google Scholar
  7. Grevesse N., Noels A., 1993, in: Origin and evolution of the elements. International Symposium of the 60 th birthday of H. Reeves Paris 1992 Eds Prantzos N. Vangioni-Flam, Casse M. Cambridge University Press, in pressGoogle Scholar
  8. Iglesias C., Rogers F.J., Wilson B.G., 1992, Astrophys. J., 397, 717CrossRefADSGoogle Scholar
  9. Kurucz, R.L., 1991, in Stellar atmospheres: Beyond Classical Models, Nato Asi Series C, Vol 341, Eds L. Crivellary, I.Hubeney, D.G. Hummer, Dordrecht.Google Scholar
  10. Morel P., Van't Veer C., Provost J., Berthomieu G., Castelli F., Cayrel R., Goupil M.J., Lebreton Y., 1994, Astron. Astrophys., 286, 91ADSGoogle Scholar
  11. Noels A., 1993, private communicationGoogle Scholar
  12. Toutain Th., Fröhlich C., 1992, Astron. Astrophys., 257, 287–297ADSGoogle Scholar
  13. Turck-Chièze S., Lopes I., 1993, Astrophys. J., 408, 347CrossRefADSGoogle Scholar

Copyright information

© Springer-Verlag 1995

Authors and Affiliations

  • P. Morel
    • 1
  • G. Berthomieu
    • 1
  • J. Provost
    • 1
  • Y. Lebreton
    • 2
  1. 1.Département CassiniURA CNRS 1362, Observatoire de la Côte d’AzurNice Cedex 4France
  2. 2.Observatoire de ParisDASGAL, URA CNRS 335Meudon Principal CedexFrance

Personalised recommendations