Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-26T04:34:16.917Z Has data issue: false hasContentIssue false
  • English
  • Français

Internal Solar rotation

Published online by Cambridge University Press:  25 May 2016

Takashi Sekii
Takashi Sekii*
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The rotation of the sun affects the wave propagation in the solar cavity. The measurement of the effect can be used to infer the internal rotation of the sun, and indeed much of what we know today about the dynamics of the solar interior has been derived from observation and interpretation of the rotationally induced splitting of solar p-mode frequencies. Inversion has proven to be a very powerful tool in such investigations, and will remain at the centre of our effort in studying solar rotation from helioseimic data. Study of the flow inside the sun is not only important in its own right but is vital for improving our understanding of solar activity and its cycle. Now that both GONG and SOHO are operational and are accumulating data, there is no doubt that we are about to learn a great deal more about the dynamical structure of our own star.

Type
Part II: Internal structure and rotation. Seismic inversions
Information
Symposium - International Astronomical Union , Volume 181: Sounding Solar and Stellar Interiors , 1997 , pp. 189 - 202
Copyright
Copyright © Kluwer 1997 

References

Backus, G. and Gilbert, F. (1968) Geophys. J. Roy. Astron. Soc. 16, 169.Google Scholar
Backus, G. and Gilbert, F. (1970) Phil. Trans. Roy. Soc. London, Ser. A 266, 123.Google Scholar
Chang, H.-Y., Gough, D.O. and Sekii, T. (1996), this conference (poster book).Google Scholar
Chaplin, W.J., Elsworth, Y., Howe, R., Isaak, G.R., McLeod, C.P., Miller, B.A. and New, R. (1996) MNRAS 280, 849.Google Scholar
Christensen-Dalsgaard, J., Schou, and Thompson, M.J. (1990) MNRAS 242, 353.Google Scholar
Christensen-Dalsgaard, J., Larsen, R.M., Schou, and Thompson, M.J. (1995) in GONG 1994: Helio- and Astero-Seismology from Earth and Space, the Conference Series of the Astronomical Society of the Pacific, ed Ulrich, R. K. (the Astronomical Society of the Pacific, San Francisco), 70.Google Scholar
Corbard, T., Berthomieu, G., Gonczi, G., Provost, J. and Morel, P. (1995) in The 4th SOHO Workshop, Helioseismology, ed. Battrick, B. (ESA Publication Division, Noordwijk), 289.Google Scholar
Duvall, T.L. Jr. et al. (1996) these proceedings.Google Scholar
Gough, D.O. (1996) in The Structure of the Sun, ed Roca Cortés, T. (Cambridge University Press), 141.Google Scholar
Gough, D.O. and Toomre, J. (1993) GONG Report No. 11.Google Scholar
Gough, D.O. and Sekii, T. (1996) this conference (poster book).Google Scholar
Hansen, C.J., Cox, J.P. and van Horn, H.M. (1977) ApJ 217, 151.Google Scholar
Harvey, J.W. et al. (1996) Science 272, 1284.Google Scholar
Korzennik, S.G., Thompson, M.J., Toomre, J. and the GONG internal rotation team (1996) these proceedings.Google Scholar
Kosovichev, A.G. and Duvall, T.L. Jr. (1996) in Solar Convection and Oscillations and their Relationship eds. Pijpers, F.P., Christensen-Dalsgaard, J. and Rosenthal, C.S. (Kluwer Academic), in press.Google Scholar
Kosovichev, A.G. et al. (1996) Sol. Phys., submitted.Google Scholar
Lazrek, M et al. (1996) Sol. Phys., 166, 1.Google Scholar
Pallé, P.L. (1996) these proceedings.Google Scholar
Phillips, D.L. (1962) J. Ass. Comput. Mach. 9, 84.Google Scholar
Pijpers, F.P. and Thompson, M.J. (1992) A&A 262, L33.Google Scholar
Pijpers, F.P. and Thompson, M.J. (1996) MNRAS 279, 498.Google Scholar
Ritzwoller, M.H. and Lavely, E.M. (1991) ApJ 369, 557.Google Scholar
Schou, J. (1991) in Challenges to theories of the structure of moderate-mass stars, eds. Gough, D.O. and Toomre, J. (Springer, Heidelberg).Google Scholar
Sekii, T. 1990) in Progress of Seismology of the Sun and Stars, eds. Osaki, Y. and Shibahashi, H. (Springer-Verlag, Berlin), 337.CrossRefGoogle Scholar
Sekii, T. (1991) PASJ, 43, 381.Google Scholar
Sekii, T. (1993a) in GONG1992: Seismic Investigation of the Sun and Stars, the Conference Series of the Astronomical Society of the Pacific, ed Brown, T.M. (the Astronomical Society of the Pacific, San Francisco), 237.Google Scholar
Sekii, T. (1993b) MNRAS 264, 1018.Google Scholar
Sekii, T. (1995) in The 4th SOHO Workshop, Helioseismology, ed. Battrick, B. (ESA Publication Division, Noordwijk), 285.Google Scholar
Spiegel, E.A. and Zahn, J.-P. (1992) A&A, 265, 106.Google Scholar
Thompson, M.J. el al. (1996) Science 272, 1300.Google Scholar
Tomczyk, S., Schou, J. and Thompson, M.J. (1995) ApJ, L57.Google Scholar
Tikhonov, A.N. (1963) Sov. Maths-Dokl. 4, 1035.Google Scholar
Twomey, S. (1963) J. Ass. Comput. Mach. 10, 97.Google Scholar