Abstract
We discuss the choice of the difference scheme and of the variables. We also show that a slight modification to the usual difference method allows a significant increase of the accuracy and the computation of, a solar model with a reasonable number of meshpoints.
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References
Christensen-Dalsgaard, J., 1988, Computation procedure for GONG solar models
Henyey, L.G., Forbes J.E. and Gould, N.L., 1964, Astrophys. J. 139, 306
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© 1991 Springer-Verlag
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Gabriel, M. (1991). Accuracy tests for the computation of solar models. In: Gough, D., Toomre, J. (eds) Challenges to Theories of the Structure of Moderate-Mass Stars. Lecture Notes in Physics, vol 388. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-54420-8_50
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DOI: https://doi.org/10.1007/3-540-54420-8_50
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Online ISBN: 978-3-540-38355-0
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