Abstract
The SSM, invented in early nineteen sixties, remains a useful construction. There are now much larger number of its predictions that may be compared with observations than when it was first introduced. Seismic sounding based on oscillations frequencies provides the best test of the physical input for modelling stellar evolution. The results of the test must be viewed as a support for the standard theory of stellar evolution. However, significant differences in the sound-speed, photospheric He abundance, and other parameters between the Sun and the current models remain. Shortcomings in the EOS and in treatment of convection have been revealed. The differences in the sound-speed in the radiative interior may be explained by small opacity errors but other explanations are possible. Results of seismic sounding support the idea that the element mixing in the outer part of the radiative interior occurred during a significant fraction of the Sun's life. Such mixing is considered as a possible explanation of the deficit of lithium. The shortcomings of SSM cannot explain the deficits of measured neutrino fluxes.
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References
Antia, H.M.: 1998, ‘Estimate of solar radius from f-mode frequencies', Astron. Astrophys. 330, 336–340.
Bahcall, J.N. and Bethe, H.A.: 1990, ‘A solution of the Solar-Neutrino Problem', Phys. Rev. Lett. 65, 2233–2238.
Basu, S.: 1998, ‘Effects of Errors in the Solar Radius on Helioseismic Inferences', Month. Not. Roy astron. Soc., in the press.
Basu, S., Christensen-Dalsgaard, J.: 1997, ‘Equation of state and helioseismic inversions', Astron Astrophys. 337, L5-L8.
Canuto, V.: 1990, ‘The mixing length parameter α', Astron. Astrophys. 227, 282–284.
Christensen-Dalsgaard, J. et al.: 1996, ‘The current state of solar modelling', Science 272, 1286–1292.
Christensen-Dalsgaard, J.: 1998, ‘The “standard” Sun', Space Sci. Rev., this volume.
Christensen-Dalsgaard, J., Däppen, W.: 1992, ‘Solar oscillations and equation of state', Astron. Astrophys. Rev. 4, 267–361.
Däppen, W.: 1998, ‘Microphysics: equation of state', Space Sci. Rev., this volume.
Däppen, W., Mihalas, D., Hummer, D.G. and Mihalas, B.: 1988, ‘The equation of state for stellar envelopes. III. Thermodynamical quantities’ Astrophys. J. 332, 261–270.
Dziembowski, W.A., Goode, P.R., Pamyatnykh, A.A. and Sienkiewicz, R.: 1994, ‘Seismic Model on the Sun's Interior', Astrophys. J. 432, 417–426.
Dziembowski, W.A., Pamyatnykh, A.A. and Sienkiewicz, R.: 1992, ‘Seismological Tests of Standard Solar Models Calculated with New Opacities', Acta Astronomica 42, 5–15.
Elsworth, Y., Howe, R., Isaak, G.R., McLeod, C.P., Miller, B.A., New, R., Speake, C.C. and Wheeler, S.J.: 1994, ‘Solar p-mode frequencies and their dependence on solar activity: Recent results from the BISON network', Astrophys. J. 434, 801–806.
Gough, D.O., et al.: 1996, ‘The Seismic Structure of the Sun', Science 272, 1296–1299.
Libbrecht, K.G., Woodard, M.F. and Kaufman, J.M.: 1990, ‘Frequencies of solar oscillations', Astrophys. J. Suppl. 74, 1129–1149.
Rhodes, E.J., Kosovichev, A.G., Schou, J., Scherrer, P.H. and Reiter, J.: 1997, Measurements of Frequencies of Solar Oscillations from the MDI Medium-ℓ' Program, Solar Phys. 175, 287–310.
Richard, O., Vauclair, S., Charbonnel, C. and Dziembowski, W.A.: 1996, ‘New Solar Models Including Helioseismological Constraints and Light Element Depletion', Astron. Astrophys. 312, 1000–1013.
Richard, O., Dziembowski, W.A., Sienkiewicz, R. and Goode, P.R.: 1998,’ On the Accuracy of Helioseismic Determination of Solar Helium Abundance', Astronomy and Astrophysics, submitted.
Rogers, F.J., Swenson, F.J. and Iglesias, C.A.: 1996, ‘OPAL equation-of-state tables for astrophysical applications', Astrophys. J. 456, 902–908.
Rogers, F.J. and Iglesias, C.A.: 1998, ‘Opacity of stellar matter', Space Sci. Rev., this volume.
Schou, J., Kosovichev, A.G., Goode, P.R., and Dziembowski, W.A.: 1997, ‘Determination of the Sun's Seismic Radius from SOHO/MDI', Astrophys. J. Lett. 489, L197–201.
Suzuki, Y.: 1998, ‘Solar neutrinos', Space Sci. Rev., this volume.
Tripathy, S.C., Basu, S. and Christensen-Dalsgaard, J.: 1997, ‘Helioseismic determination of opacity correction', in J. Provost and F.-X. Schmider (eds.), Sounding Solar and Stellar Interiors, (Nice), poster.
Turck-Chièze, S. and Brun, A.S.: 1998, ‘Spatial Seismic Constraints on Solar Neutrino Predictions', in W. Hampel (ed.), Fourth International Neutrino Conference, Heidelberg, in the press.
Vauclair, S.: 1998, ‘Element settling in the solar interior', Space Sci. Rev., this volume.
Weiss, A. and Schlattl, H.: 1998, ‘The age of the most nearby star', Astronomy and Astrophysics 332, 215–223.
Zahn, J.-P.: 1998, ‘Macroscopic transport', Space Sci. Rev., this volume.
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Dziembowski, W. Shortcomings of the Standard Solar Model. Space Science Reviews 85, 37–48 (1998). https://doi.org/10.1023/A:1005172200165
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DOI: https://doi.org/10.1023/A:1005172200165