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Seismology of Solar Internal Rotation

Published online by Cambridge University Press:  30 March 2016

Takashi Sekii
Takashi Sekii*
Affiliation:
Solar Physics Division, National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, JAPAN

Abstract

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Helioseismologists have been highly successful in revealing how the solar interior differentially rotates, through observations of rotationally split eigen p modes of the Sun. What we currently know about the internal rotation of the Sun is reviewed, and outstanding issues are discussed.

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 424 - 427
Copyright
Copyright © Astronomical Society of Pacific 2005

References

Aerts, C. et al. 2003, Science, 300, 1926 CrossRefGoogle Scholar
Choudhuri, A. R. 1990, ApJ, 355, 733 CrossRefGoogle Scholar
Dikpati, M., & Charbonneau, P. 1999, ApJ, 518, 508 CrossRefGoogle Scholar
Elliott, J. R. 2003, in Stellar Astrophysical Fluid Dynamics, ed. Thompson, M. J. & Christensen-Dalsgaard, J. (Cambridge University Press), 315 CrossRefGoogle Scholar
Garaud, P. 2003, in Stellar Astrophysical Fluid Dynamics, ed. Thompson, M. J. & Christensen-Dalsgaard, J. (Cambridge, Cambridge University Press), 131 CrossRefGoogle Scholar
Giles, P. M. et al. 1997, Nature, 390, 52 Google Scholar
Gizon, L., et al. 2001, in Solar Encounter: The First Solar Orbitor Workshop, ed. Battrick, B. & Sawaya-Lacoste, H. (Noordwijk, ESA), 227 Google Scholar
Glatzmaier, G. 1985, ApJ, 291, 300 CrossRefGoogle Scholar
Gough, D., & Mclntyre, M. E. 1998, Nature, 394, 755 CrossRefGoogle Scholar
Gough, D. O., & Sekii, T. 1998, in Sounding Solar and Steller Interiors, ed. Berthomieu, G., Provost, J. and Schmider, F. X. (Nice, Observatoire de la Côte d’ Azur), 93 Google Scholar
Gough, D. O. et al. 1996, Science, 272, 1296 CrossRefGoogle Scholar
Hathaway, D. et al. 1996, Science, 272, 1306 CrossRefGoogle Scholar
Howe, R. et al. 2000, Science, 287, 2456 CrossRefGoogle Scholar
Kawaler, S. D., Sekii, T., & Gough, D. O. 1999, ApJ, 516, 349 CrossRefGoogle Scholar
Nandy, D., & Choudhuri, A. R. 2002, Science, 296, 1671 CrossRefGoogle Scholar
Parker, E. N. 1993, ApJ, 408, 707 CrossRefGoogle Scholar
Schou, J. et al. 1998, ApJ, 505, 390 CrossRefGoogle Scholar
Sekii, T. 1997, in Sounding Solar and Steller Interiors, ed. Berthomieu, G., Provost, J. & Schmider, F. X. (Dordrecht, Kluwer Academic), 189 CrossRefGoogle Scholar
Sekii, T. 2003, in Stellar Astrophysical Fluid Dynamics, ed. Thompson, M. J. & Christensen-Dalsgaard, J. (Cambridge, Cambridge University Press), 263 CrossRefGoogle Scholar
Spiegel, E. A., & Zahn, J.-P. 1992, A&A, 265, 106 Google Scholar
Thompson, M. J. 1996, Science, 272, 1300 CrossRefGoogle Scholar
Winget, D. E. et al. 1991, ApJ, 378, 326 CrossRefGoogle Scholar
Winget, D. E. et al. 1994, ApJ, 430, 839 CrossRefGoogle Scholar