Modelling the solar interior

Details Modelling the solar interior Modelling the solar interior

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..919....1b&link_type=abstract

KODAI SCHOOL ON SOLAR PHYSICS. AIP Conference Proceedings, Volume 919, pp. 1-23 (2007).

Physics

5

Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Solar Interior

Scientific paper

The equations of stellar structure and evolution need to be solved to model the interior of the Sun. Modelling the Sun is, however, slightly more complicated than modelling other stars since we have more observational constraints for the Sun than for other stars. In this article we discuss the basics of modelling the interior structure of the Sun. We also discuss the inputs needed to construct such a model, and how we test whether the resulting solar model is correct.

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