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

Timothy R. Bedding; Allan S. Brun; Jørgen Christensen-Dalsgaard; Ashley Crouch; Peter De Cat; Raphael A. García; Laurent Gizon; Frank Hill; Hans Kjeldsen; John W. Leibacher; Jean Pierre Maillard; S. Mathis; M. Cristina Rabello-Soares; Jean Pierre Rozelot; Matthias Rempel; Ian W. Roxburgh; Réza Samadi; Suzanne Talon; Michael J. Thompson

doi:10.1017/S1743921307011635

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

Timothy R. Bedding
, Allan S. Brun
, Jørgen Christensen-Dalsgaard
, Ashley Crouch
, Peter De Cat
, Raphael A. García
, Laurent Gizon
, Frank Hill
, Hans Kjeldsen
, John W. Leibacher
, Jean Pierre Maillard
, S. Mathis
, M. Cristina Rabello-Soares
, Jean Pierre Rozelot
, Matthias Rempel
, Ian W. Roxburgh
, Réza Samadi
, Suzanne Talon
, Michael J. Thompson

HAO Administrative Office

University of Sydney
CEA Saclay
Aarhus University
Canadian Space Agency
Royal Observatory of Belgium
Max Planck Institute for Solar System Research
National Optical Astronomy Observatory
Institut d'Astrophysique Spatiale
LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique
Institut d’Astrophysique de Paris
Stanford University
Université Côte d'Azur
Queen Mary University of London
University of Montreal
University of Sheffield

Research output: Contribution to journal › Article › peer-review

Abstract

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.

Original language	English
Pages (from-to)	491-516
Number of pages	26
Journal	Proceedings of the International Astronomical Union
Volume	2
Issue number	14
DOIs	https://doi.org/10.1017/S1743921307011635
State	Published - Aug 2006

Keywords

Space vehicles: instruments
Stars: interiors
Stars: oscillations (including pulsations)
Stars: rotation
Sun: helioseismology
Sun: interior
Sun: rotation

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Bedding, T. R., Brun, A. S., Christensen-Dalsgaard, J., Crouch, A., De Cat, P., García, R. A., Gizon, L., Hill, F., Kjeldsen, H., Leibacher, J. W., Maillard, J. P., Mathis, S., Rabello-Soares, M. C., Rozelot, J. P., Rempel, M., Roxburgh, I. W., Samadi, R., Talon, S., & Thompson, M. J. (2006). Joint Discussion 17 Highlights of recent progress in the seismology of the Sun and Sun-like stars. Proceedings of the International Astronomical Union, 2(14), 491-516. https://doi.org/10.1017/S1743921307011635

@article{19373387ad094d4aa8eb01fbc4afba7d,

title = "Joint Discussion 17 Highlights of recent progress in the seismology of the Sun and Sun-like stars",

abstract = "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.",

keywords = "Space vehicles: instruments, Stars: interiors, Stars: oscillations (including pulsations), Stars: rotation, Sun: helioseismology, Sun: interior, Sun: rotation",

author = "Bedding, \{Timothy R.\} and Brun, \{Allan S.\} and J{\o}rgen Christensen-Dalsgaard and Ashley Crouch and \{De Cat\}, Peter and Garc{\'i}a, \{Raphael A.\} and Laurent Gizon and Frank Hill and Hans Kjeldsen and Leibacher, \{John W.\} and Maillard, \{Jean Pierre\} and S. Mathis and Rabello-Soares, \{M. Cristina\} and Rozelot, \{Jean Pierre\} and Matthias Rempel and Roxburgh, \{Ian W.\} and R{\'e}za Samadi and Suzanne Talon and Thompson, \{Michael J.\}",

year = "2006",

month = aug,

doi = "10.1017/S1743921307011635",

language = "English",

volume = "2",

pages = "491--516",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

number = "14",

}

Bedding, TR, Brun, AS, Christensen-Dalsgaard, J, Crouch, A, De Cat, P, García, RA, Gizon, L, Hill, F, Kjeldsen, H, Leibacher, JW, Maillard, JP, Mathis, S, Rabello-Soares, MC, Rozelot, JP, Rempel, M, Roxburgh, IW, Samadi, R, Talon, S & Thompson, MJ 2006, 'Joint Discussion 17 Highlights of recent progress in the seismology of the Sun and Sun-like stars', Proceedings of the International Astronomical Union, vol. 2, no. 14, pp. 491-516. https://doi.org/10.1017/S1743921307011635

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.

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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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 -

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

Abstract

Keywords

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