Table 6
Values of observational constraints used to produce each calibrated solar models.
| Name | Notation | Value [cgs] | |||||||
|---|---|---|---|---|---|---|---|---|---|
| Age | Age | 4570 [Myrs] | |||||||
| Effective temperature | Teff | 5772 ± 1 (1) | |||||||
| Luminosity | L | 3.828 · 1033 ± 1028 (1) | |||||||
| Surface metal to hydrogen ratio | (Z/X)s | 0.0187 ± 9 · 10−4 (2) | |||||||
| Acoustic travel-time | Tcz | 1422 ± 20 (3, 4) | |||||||
| Logarithm of surface 7Li abundance | log ϵLi,s | 0.96 ± 0.06 (2) | |||||||
| Surface angular velocity | Ωs | 2.86 ± 0.01 (5) | |||||||
Notes. (1) Prša et al. (2016); (2) Asplund et al. (2021); log ϵLi,s = log(NLi/NH) + 12; (3) Roxburgh (2009); Deal et al. (2023); (5) Solar surface angular velocity varies with latitude and moment of the solar cycle (e.g. Beck 2000). The value here is chosen within a range of usual values of equatorial Ωs,⊙.
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