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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

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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.

Information

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 

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