The solar photospheric silicon abundance according to CO5BOLD - Investigating line broadening, magnetic fields, and model effects

Open Access

Fig. A.3

LINFOR3D + CO⁵BOLD msc600 model model syntheses (red lines) fit to BALDER + STAGGER (black points). Green lines show residuals increased by a factor of 10. The mean abundance as derived by the CO⁵BOLD fit is 7.51 ± 0.01.

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