Hostname: page-component-cd9895bd7-p9bg8 Total loading time: 0 Render date: 2024-12-21T17:42:14.060Z Has data issue: false hasContentIssue false
  • English
  • Français

Structure inversions with the VIRGO data

Published online by Cambridge University Press:  25 May 2016

Thierry Appourchaux ,
Takashi Sekii ,
Douglas Gough ,
Umin Lee ,
Christoph Wehrli  and
The VIRGO Team
Thierry Appourchaux
Affiliation:
Space Science Department, ESTEC, NL-2200 AG Noordwijk, The Netherlands
Takashi Sekii
Affiliation:
Institute of Astronomy, University of Cambridge, Cambridge CB3 0HA, UK
Douglas Gough
Affiliation:
Institute of Astronomy, University of Cambridge, Cambridge CB3 0HA, UK Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge CB3 9EW, UK
Umin Lee
Affiliation:
Astronomical Institute, Tohoku University Sendai, Miyagi 980, Japan
Christoph Wehrli
Affiliation:
Physikalisch-Meteorologisches Observatorium Davos, World Radiation Center, CH-7260 Davos Dorf, Switzerland

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.

The p-mode frequencies obtained by the VIRGO instrument have been inverted to derive the solar core structure. Two sets of frequencies have been used in the inversions. The sets are derived from different time series (the second containing the first), using different procedures for fitting the spectra. The influence of the correlations between the p-mode frequencies has been implemented in the inversion procedure. The two data sets are in good agreement with each other, and show no evidence that the sun is significantly different from the latest available standard solar model.

Type
Part II: Internal structure and rotation. Seismic inversions
Information
Symposium - International Astronomical Union , Volume 181: Sounding Solar and Stellar Interiors , 1997 , pp. 159 - 166
Copyright
Copyright © Kluwer 1997 

References

Appourchaux, T., Andersen, B.N., Fröhlich, C., Jiménez, A., Telljohan, U., Wehrli, C. (1997) Submitted to Solar Phys. Google Scholar
Appourchaux, T., Telljohann, U., Martin, D., Lévêque, S. and Fleur, J. (1995a) in Fourth SOHO workshop on helioseismology, Domingo, V. and Hoeksema, T. eds., ESA SP-376, p. 359.Google Scholar
Appourchaux, T., Toutain, T., Telljohann, U., Jiménez, A., Rabello-Soares, M.C., Andersen, B.N. and Jones, A.R. (1995b) Astron. Astrophys., 294, L13.Google Scholar
Appourchaux, T., Toutain, T., Telljohann, U., Jiménez, A., Rabello-Soares, M.C., Andersen, B.N. and Jones, A.R. (1995c) in Fourth SOHO workshop on helioseismology, Domingo, V. and Hoeksema, T. eds., ESA SP-376, p. 265.Google Scholar
Christensen-Dalsgaard, et al. (1996) Science, 272, 1286.Google Scholar
Däppen, W., Gough, D.O., Kosovichev, A.G. and Thompson, M.J. (1991) in Challenges to Theories of the Structure of Moderate-Mass Stars, Gough, D.O. & Toomre, J. eds., Springer Verlag, Berlin, p. 111.CrossRefGoogle Scholar
Fröhlich, C. and the VIRGO team (1997) Submitted to Solar Phys .Google Scholar
Gough, D.O. (1995) in Fourth SOHO workshop on helioseismology, Domingo, V. and Hoeksema, T. eds., ESA SP-376, p. 249.Google Scholar
Gough, D.O. (1996) in The structure of the Sun, Roca Cortés, T. & Sánchez, F. eds., Cambridge University Press, p 141.Google Scholar
Rabello-Soares, M.C. (1996) Helioseismological study of the solar interior, , .Google Scholar
Rabello-Soares, M.C., Roca-Cortes, T., Jiménez, A., Appourchaux, T. and Eff-Darwich, . (1996) Submitted to Astrophys. J .Google Scholar
Schou, J. (1992) On the analysis of helioseismic data, , .Google Scholar
Tomczyk, S., Schou, J. and Thompson, M.J. (1996) Astrophys. J., 448, L57.Google Scholar