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The seismic structure of the Sun from GONG

Published online by Cambridge University Press:  25 May 2016

E. Anderson ,
H.M. Antia ,
S. Basu ,
B. Chaboyer ,
S.M. Chitre ,
J. Christensen-Dalsgaard ,
A. Eff-Darwich ,
J.R. Elliott ,
P.M. Giles  and
D.O. Gough
...Show all authors
E. Anderson
Affiliation:
National Solar Observatory, Tucson, Arizona, USA
H.M. Antia
Affiliation:
Tata Institute of Fundamental Research, Bombay, India
S. Basu
Affiliation:
Theoretical Astrophysics Center, Danish National Research Foundation
B. Chaboyer
Affiliation:
Canadian Institute for Theoretical Astrophysics, Toronto, Canada
S.M. Chitre
Affiliation:
Tata Institute of Fundamental Research, Bombay, India
J. Christensen-Dalsgaard
Affiliation:
Theoretical Astrophysics Center, Danish National Research Foundation Institute of Physics and Astronomy, Aarhus University, Denmark
A. Eff-Darwich
Affiliation:
Center for Astrophysics, Cambridge, Massachusetts, USA
J.R. Elliott
Affiliation:
JILA, Boulder, Colorado, USA
P.M. Giles
Affiliation:
HEPL, Stanford University, California, USA
D.O. Gough
Affiliation:
Institute of Astronomy, University of Cambridge, UK DAMTP, University of Cambridge, UK
J.A. Guzik
Affiliation:
Los Alamos National Laboratory, New Mexico, USA
J.W. Harvey
Affiliation:
National Solar Observatory, Tucson, Arizona, USA
F. Hill
Affiliation:
National Solar Observatory, Tucson, Arizona, USA
J.W. Leibacher
Affiliation:
National Solar Observatory, Tucson, Arizona, USA
A.G. Kosovichev
Affiliation:
HEPL, Stanford University, California, USA
M.J.P.F.G. Monteiro
Affiliation:
University of Porto, Portugal
O. Richard
Affiliation:
Observatoire Midi-Pyrénées, Toulouse, France
T. Sekii
Affiliation:
Institute of Astronomy, University of Cambridge, UK
H. Shibahashi
Affiliation:
University of Tokyo, Japan
M. Takata
Affiliation:
University of Tokyo, Japan
M.J. Thompson
Affiliation:
Queen Mary & Westfield College, University of London, UK
J. Toomre
Affiliation:
JILA, Boulder, Colorado, USA
S. Vauclair
Affiliation:
Observatoire Midi-Pyrénées, Toulouse, France
S.V. Vorontsov
Affiliation:
Queen Mary & Westfield College, University of London, UK

Extract

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This paper is an interim report of our inferences about the hydrostatic structure of the Sun, following the first report of the GONG team in Science (Gough et al., 1996). That work confirms that the spherically averaged structure of the Sun is more or less in agreement with current standard solar models. However, there remain some significant deviations which we regard as important clues to the existence of dynamical phenomena which are not taken into account in standard solar modelling.

Type
Part II: Internal structure and rotation. Seismic inversions
Information
Symposium - International Astronomical Union , Volume 181: Sounding Solar and Stellar Interiors , 1997 , pp. 151 - 158
Copyright
Copyright © Kluwer 1997 

References

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