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Joint Discussion 17 Highlights of recent progress in the seismology of the Sun and Sun-like stars

Published online by Cambridge University Press:  01 August 2006

Timothy R. Bedding
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia email: bedding@physics.usyd.edu.au
Allan S. Brun
Affiliation:
DSM/DAPNIA/Service d'Astrophysique & UMR AIM 7158, CEA Saclay, F-91191 Gif-sur-Yvette, France email: sacha.brun@cea.fr, rafael.garcia@cea.fr, stephane.mathis@cea.fr
Jørgen Christensen-Dalsgaard
Affiliation:
Institut for Fysik og Astronomi, Aarhus Universitet, DK-8000 Aarhus C, Denmark email: jcd@phys.au.dk, hans@phys.au.dk
Ashley Crouch
Affiliation:
Canadian Space Agency, Longueuil, QC, J3Y 8Y9, Canada email: ash@astro.umontreal.ca
Peter De Cat
Affiliation:
Royal Observatory Belgium, Avenue Circulaire 3, B-1180 Brussels, Belgium email: peter@oma.be
Raphael A. García
Affiliation:
DSM/DAPNIA/Service d'Astrophysique & UMR AIM 7158, CEA Saclay, F-91191 Gif-sur-Yvette, France email: sacha.brun@cea.fr, rafael.garcia@cea.fr, stephane.mathis@cea.fr
Laurent Gizon
Affiliation:
Max-Planck-Institut für Sonnensystemforschung, D-37191 Katlenburg-Lindau, Germany email: gizon@linmpi.mpg.de
Frank Hill
Affiliation:
National Solar Observatory, NOAO, 950 N Cherry Ave, Tucson, AZ 85719-4933, USA email: fhill@nso.edu, jleibacher@nso.edu
Hans Kjeldsen
Affiliation:
Institut for Fysik og Astronomi, Aarhus Universitet, DK-8000 Aarhus C, Denmark email: jcd@phys.au.dk, hans@phys.au.dk
John W. Leibacher
Affiliation:
National Solar Observatory, NOAO, 950 N Cherry Ave, Tucson, AZ 85719-4933, USA email: fhill@nso.edu, jleibacher@nso.edu Institut d'Astrophysique Spatiale, Centre Universitaire d'Orsay, F-91405 Orsay, France LESIA, Observatoire de Paris, CNRS UMR 8109, F-92195 Meudon, France email: reza.samadi@obspm.fr
Jean-Pierre Maillard
Affiliation:
Institut d'Astrophysique de Paris, 98bis Bd Arago, F-75014 Paris, France email: maillard@iap.fr
S. Mathis
Affiliation:
Royal Observatory Belgium, Avenue Circulaire 3, B-1180 Brussels, Belgium email: peter@oma.be
M. Cristina Rabello-Soares
Affiliation:
Hansen Experimental Physics Laboratory, Stanford University, CA 94305, USA email: csoares@sun.stanford.edu
Jean-Pierre Rozelot
Affiliation:
Observatoire de la Côte d'Azur, GEMINI, F-06130Grasse, France email: jean-pierre.rozelot@obs-azur.fr
Matthias Rempel
Affiliation:
High Altitude Observatory, NCAR, PO Box 3000, Boulder, CO 80307-3000, USA email: rempel@hao.ucar.edu
Ian W. Roxburgh
Affiliation:
Astronomy Unit, Queen Mary, University of London, London E1 4NS, UK email: i.w.roxburgh@qmul.ac.uk
Réza Samadi
Affiliation:
LESIA, Observatoire de Paris, CNRS UMR 8109, F-92195 Meudon, France email: reza.samadi@obspm.fr
Suzanne Talon
Affiliation:
Département de Physique, Université de Montréal, QC H3C 3J7, Canada email: talon@astro.umontreal.ca
Michael J. Thompson
Affiliation:
SP2RC, Department of Applied Mathematics, University of Sheffield, Sheffield S3 7RH, UK email: michael.thompson@sheffield.ac.uk
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Abstract

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The seismology and physics of localized structures beneath the surface of the Sun takes on a special significance with the completion in 2006 of a solar cycle of observations by the ground-based Global Oscillation Network Group (GONG) and by the instruments on board the Solar and Heliospheric Observatory (SOHO). Of course, the spatially unresolved Birmingham Solar Oscillation Network (BiSON) has been observing for even longer. At the same time, the testing of models of stellar structure moves into high gear with the extension of deep probes from the Sun to other solar-like stars and other multi-mode pulsators, with ever-improving observations made from the ground, the success of the MOST satellite, and the recently launched CoRoT satellite. Here we report the current state of the two closely related and rapidly developing fields of helio- and asteroseimology.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

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