Hostname: page-component-7479d7b7d-qs9v7 Total loading time: 0 Render date: 2024-07-13T17:03:33.066Z Has data issue: false hasContentIssue false
  • English
  • Français

Seismological Constraints on Convective Penetration in the Sun

Published online by Cambridge University Press:  12 April 2016

G. Berthomieu ,
P. Morel ,
J. Provost  and
J.-P. Zahn
G. Berthomieu
Affiliation:
Cassini, URA CNRS 1362, Observatoire de la Côte d’Azur, Nice
P. Morel
Affiliation:
Cassini, URA CNRS 1362, Observatoire de la Côte d’Azur, Nice
J. Provost
Affiliation:
Cassini, URA CNRS 1362, Observatoire de la Côte d’Azur, Nice
J.-P. Zahn
Affiliation:
Observatoire Midi-Pyrénées, Toulouse Columbia University, New York

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Penetrative convection is expected below stellar convection sones, where it should achieve a nearly adiabatic stratification. A theoretical prediction of the penetration depth has been recently made by Zahn (1991) which includes an arbitrary parameter ζ depending on the properties of the convective motions. We use the helioseismological constraints to calibrate the value of this parameter.

Type
I. Setting the stage: Sun, Stars Galaxies and the Universe
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 60 - 62
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Anders, E., Grevesse, N.: 1989, Geochim. Cosmochim. Acta 53, 197 CrossRefGoogle Scholar
Gough, D.O.: 1991, in Progress of seismology of the sun and stars, Eds Shibahashi H., Osaki Y., Springer Verlag, p 283–318 Google Scholar
Iglesias, C.A., Rogers, F.J.: 1991 Astrophys. J. 371, 408–417 CrossRefGoogle Scholar
Libbrecht, K.G., Woodard, M.F., Kaufman, J.M.: 1990, Astrophys. J. Supp. 74, 1129 CrossRefGoogle Scholar
Zahn, J.P.: 1991, Astron. Astrophys. 252 179–188 Google Scholar