Hostname: page-component-68945f75b7-tmfhh Total loading time: 0 Render date: 2024-08-05T21:20:58.550Z Has data issue: false hasContentIssue false
  • English
  • Français

Inversion Methods

Published online by Cambridge University Press:  08 February 2017

M.J. Thompson
M.J. Thompson*
Affiliation:
Astronomy Unit, School of Mathematical Sciences, Queen Mary & Westfield College, London, E1 4NS, England

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.

I want to start by addressing the question, ‘What is inversion?’ My answer would be that inversion is the process of going from data to making inferences about the object under study. In the case of helioseismology, the data at the present time are principally the mode frequencies, and the object under study is the solar interior.

Type
III. Large-Scale Structure of the Sun
Information
Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 125 - 134
Copyright
Copyright © Kluwer 1998 

References

Brodsky, M. A. & Vorontsov, S. V., 1988. In Proc. IAU Symposium No 123, Advances in helio- and asteroseismology, p. 137–140, eds Christensen-Dalsgaard, J. & Frandsen, S., Reidel, Dordrecht.CrossRefGoogle Scholar
Charbonneau, P., Tomczyk, S., Schou, J. & Thompson, M. J., 1997. Astrophys. J., in press.Google Scholar
Christensen-Dalsgaard, J., Gough, D. O. & Thompson, M. J., 1991. Astrophys. J., 378, 413–437.Google Scholar
Christensen-Dalsgaard, J., Schou, J. & Thompson, M. J., 1990. Mon. Not. R. astr. Soc., 242, 353–369.CrossRefGoogle Scholar
Christensen-Dalsgaard, J., Duvall, T. L., Gough, D. O., Harvey, J. W. & Rhodes, E. J. Jr, 1985. Nature, 315, 378–382.CrossRefGoogle Scholar
Genovese, C. R., Stark, P. B. & Thompson, M. J., 1995. Astrophys. J., 443, 843–854.Google Scholar
Gough, D. O., 1984. Phil. Trans. R. Soc. London, Ser. A, 313, 27–38.Google Scholar
Gough, D. O., 1985. Solar Phys., 100, 65–99.Google Scholar
Gough, D. O., 1986. In Seismology of the Sun and the distant Stars, p. 125–140, ed. Gough, D. O., Reidel, Dordrecht.CrossRefGoogle Scholar
Gough, D. O. & Thompson, M. J., 1991. In Solar interior and atmosphere, eds Cox, A. N., Livingston, W. C. & Matthews, M., p. 519–561, Space Science Series, University of Arizona Press.Google Scholar
Howe, R. & Thompson, M. J., 1996. Mon. Not. R. astr. Soc., 281, 1385–1392.Google Scholar
Korzennik, S. G., Thompson, M. J., Toomre, J. & the GONG Internal Rotation Team, 1997. To appear in Proc. IAU Symposium 181 ‘Sounding solar and stellar interiors’ , eds Provost, J. & Schmider, F. X. (Kluwer, Dordrecht).Google Scholar
Kosovichev, A. G., 1996. Astrophys. J., 469, L61–L64.Google Scholar
Pijpers, F. P. & Thompson, M. J., 1992. Astron. Astrophys., 262, L33–L36.Google Scholar
Schou, J., Antia, H. M., Basu, S., et al., 1997a. Astrophys. J., submitted.Google Scholar
Schou, J. & the SOI Internal Rotation Team, 1997b, these proceedings.CrossRefGoogle Scholar
Shibahashi, H., 1988. In Proc. IAU Symposium No 123, Advances in helio- and asteroseismology, p. 133–136, eds Christensen-Dalsgaard, J. & Frandsen, S., Reidel, Dordrecht.CrossRefGoogle Scholar
Thompson, M. J., Toomre, J., et al., 1996. Science, 272, 1300–1305.Google Scholar
Tomczyk, S., Schou, J. & Thompson, M. J., 1995. Astrophys. J. Lett., 448, L57–L60.Google Scholar
Toutain, T., Appourchaux, T., Baudin, F., et al., 1997. Solar Phys., in press.Google Scholar