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Internal rotation and dynamics of the Sun from GONG data

Published online by Cambridge University Press:  25 May 2016

S. G. Korzennik ,
M. J. Thompson ,
J. Toomre  and
The GONG Internal Rotation Team
S. G. Korzennik
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St, Cambridge MA 02138, USA
M. J. Thompson
Affiliation:
Astronomy Unit, Queen Mary & Westfield College, Mile End Rd, London El 4NS, UK
J. Toomre
Affiliation:
Joint Institute for Laboratory Astrophysics, University of Colorado, Boulder CO 80309, USA

Extract

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We report inferences for the Sun's internal rotation from GONG months 4-10 averaged power spectra. In keeping with the international collaborative nature of the GONG project, the results presented here are based on the work of several groups around the world inverting the GONG data and sharing their results via the world-wide web. These groups are at the Observatoire de la Côte d'Azur, Nice (T. Corbard, G. Berthomieu, J. Provost); Theoretical Astrophysics Center, Aarhus (J. Christensen-Dalsgaard, F. Pijpers); Center for Astrophysics, Cambridge MA (A. Eff-Darwich, S. Korzennik); QMW, London (R. Howe, M. Thompson, in collaboration with J. Schou, Stanford); Institute of Astronomy, Cambridge (T. Sekii, D. Gough); University of Sydney (D. Burtonclay, Li Yan, P. Wilson); and Tata Institute of Fundamental Research, Bombay (H. Antia, S. Chitre).

Type
Part II: Internal structure and rotation. Seismic inversions
Information
Symposium - International Astronomical Union , Volume 181: Sounding Solar and Stellar Interiors , 1997 , pp. 211 - 218
Copyright
Copyright © Kluwer 1997 

References

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