Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-25T19:39:13.987Z Has data issue: false hasContentIssue false
  • English
  • Français

A general confrontation between solar data and solar models

Published online by Cambridge University Press:  25 May 2016

R. A. Bell  and
M. J. Tripicco
R. A. Bell
Affiliation:
Department of Astronomy University of Maryland College Park, MD 20742, USA
M. J. Tripicco
Affiliation:
Department of Astronomy University of Maryland College Park, MD 20742, USA

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.

Since its effective temperature, surface gravity and chemical composition are well established, the Sun has often been used for tests of model stellar photospheres. There are two important potential tests – firstly, comparisons of observed and calculated line spectra and, secondly, comparisons of observed and calculated fluxes. If solar model calculations can successfully reproduce both of these data sets, then it gives confidence in the quality of models of other cool stars. However, different observations of solar fluxes do not agree with one another with the precision required in testing solar models.

Type
Session V: “Next Generation Model Atmospheres”
Information
Symposium - International Astronomical Union , Volume 176: Stellar Surface Structure , 1996 , pp. 527 - 538
Copyright
Copyright © Kluwer 1996 

References

Arvesen, J.C., Griffin, R.N. Jr. and Pearson, B.D. Jr. (1969) Appl Optics , 8, 2215 (AGP) CrossRefGoogle Scholar
Bell, K.L. and Berrington, K.B. (1987) J. Phys. B. , 20, 801 CrossRefGoogle Scholar
Bell, R.A., Paltoglou, G. and Tripicco, M.J. (1994) MNRAS , 268, 771 CrossRefGoogle Scholar
Bell, R.A. and Tripicco, M.J. (1995) in IAU Joint Discussion 16, Astrophysical Application of Powerful New Atomic Databases , A.S.P. Conference Series, No. 78, ed. by Adelman, S.J. & Wiese, W.L., p. 365 Google Scholar
Bessel, M. S. (1990) PASP , 102, 1181 CrossRefGoogle Scholar
Brault, J. and Testerman, L. (1972) Kitt Peak Preliminary Solar Atlas , Kitt Peak National Observatory Google Scholar
Briley, M.M., Hesser, J.E., Bell, R.A., Bolte, M. and Smith, G.H. (1994) AJ , 108, 2183 CrossRefGoogle Scholar
Delbouille, L., Neven, L. and Roland, G. (1973) Photometric Atlas of the Solar Spectrum from $lD3000 to $lD10000 , Institut d'Astrophysique de l'Université de Liege and Observatoire Royale de Belgique Google Scholar
Dragon, J.N. and Mutschlechner, J.P. (1980) ApJ , 239, 1045 CrossRefGoogle Scholar
Dreiling, L. A. and Bell, R.A. (1980) ApJ , 241, 737 CrossRefGoogle Scholar
Gustafsson, B., Bell, R.A., Eriksson, K. and Nordlund, Å. (1975) A&A , 42, 407 Google Scholar
Gustafsson, B. and Bell, R.A. (1979) A&A , 74, 313 Google Scholar
Hayes, D.S. (1985) in IAU Symposium 111, Calibration of Fundamental Stellar Quantities , ed. Hayes, D.S., Pasinetti, L.E. & Philip, A.G.D., p. 225 Google Scholar
Holweger, H. (1970) A&A , 4, 11 Google Scholar
Kurucz, R.L. (1979) ApJS , 40, 1 CrossRefGoogle Scholar
Kurucz, R.L., Furenlid, I., Brault, J. and Testerman, J. (1984) Solar Flux Atlas from 296 to 1300 nm , National Solar Observatory, Sunspot, NM.Google Scholar
Kurucz, R.L. (1991) in Stellar Atmospheres: Beyond Classical Models , ed. Crivellari, L., Hubeny, I. & Hummer, D.G., NATO ASI Series, Kluwer, Dordrecht, p. 408.Google Scholar
Kurucz, R.L. (1992a) in The Stellar Populations of Galaxies , ed. Barbuy, B. & Renzini, A., Kluwer, Dordrecht, p. 225 CrossRefGoogle Scholar
Kurucz, R.L. (1992b) Rev. Mex. Astr. Astrof. , 23, 181 Google Scholar
Kurucz, R.L. (1993a) CD-ROM 13, ATLAS9 Stellar Atmosphere Programs and 2 km/sec Grid , Cambridge, Smithsonian Astrophysical Observatory Google Scholar
Kurucz, R.L. (1993b) CD-ROM 18, SYNTHE Spectrum Synthesis Programs and Line Data , Cambridge, Smithsonian Astrophysical Observatory Google Scholar
Labs, D. and Neckel, H. (1968) Z. Astrophys , 69, 1 Google Scholar
Labs, D. and Neckel, H. (1970) Solar Phys , 15, 79 CrossRefGoogle Scholar
Lockwood, G.W., Tug, H. and White, N.M. (1992) ApJ , 390, 668 (LTW) CrossRefGoogle Scholar
Neckel, H. and Labs, D. (1984) Solar Phys , 90, 245 (NL84) CrossRefGoogle Scholar
Stevenson, C. C. (1994) MNRAS 267, 904 CrossRefGoogle Scholar
Tripicco, M.J. and Bell, R.A. (1995) AJ (in press, Dec.) Google Scholar
Wishart, A.W. (1979) MNRAS , 187, 59P CrossRefGoogle Scholar