TY - JOUR
T1 - Joint Discussion 17 Highlights of recent progress in the seismology of the Sun and Sun-like stars
AU - Bedding, Timothy R.
AU - Brun, Allan S.
AU - Christensen-Dalsgaard, Jørgen
AU - Crouch, Ashley
AU - De Cat, Peter
AU - García, Raphael A.
AU - Gizon, Laurent
AU - Hill, Frank
AU - Kjeldsen, Hans
AU - Leibacher, John W.
AU - Maillard, Jean Pierre
AU - Mathis, S.
AU - Rabello-Soares, M. Cristina
AU - Rozelot, Jean Pierre
AU - Rempel, Matthias
AU - Roxburgh, Ian W.
AU - Samadi, Réza
AU - Talon, Suzanne
AU - Thompson, Michael J.
N1 - Copyright:
Copyright 2007 Elsevier B.V., All rights reserved.
PY - 2006/8
Y1 - 2006/8
N2 - 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.
AB - 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.
KW - Space vehicles: instruments
KW - Stars: interiors
KW - Stars: oscillations (including pulsations)
KW - Stars: rotation
KW - Sun: helioseismology
KW - Sun: interior
KW - Sun: rotation
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U2 - 10.1017/S1743921307011635
DO - 10.1017/S1743921307011635
M3 - Article
AN - SCOPUS:37049021798
SN - 1743-9213
VL - 2
SP - 491
EP - 516
JO - Proceedings of the International Astronomical Union
JF - Proceedings of the International Astronomical Union
IS - 14
ER -