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Table 1:

Atomic data of silicon lines*.

$\lambda$  [Å]
Transition $\log gf$ $\log C_6$

3905.53
$3p~^1{\rm S}^{{\rm }}_{\rm0}$- $4s~^1{\rm P}^{{\rm o}}_{\rm 1}$ -1.10 -30.917
4102.93 $3p~^1{\rm S}^{{\rm }}_{\rm0}$- $4s~^3{\rm P}^{{\rm o}}_{\rm 1}$ -2.99 -30.972
5690.43 $4s~^3{\rm P}^{{\rm o}}_{\rm 1}$- $5p~^3{\rm P}^{{\rm }}_{\rm 1}$ -1.74 -30.294
5701.11 $4s~^3{\rm P}^{{\rm o}}_{\rm 1}$- $5p~^3{\rm P}^{{\rm }}_{\rm0}$ -1.96 -30.294
5772.15 $4s~^1{\rm P}^{{\rm o}}_{\rm 1}$- $5p~^1{\rm S}^{{\rm }}_{\rm0}$ -1.62 -30.287
6142.49 $3p^3~^3{\rm D}^{{\rm o}}_{\rm 3}$- $5f~^3{\rm D}^{{\rm }}_{\rm 3}$ -1.48 -29.869
6145.05 $3p^3~^3{\rm D}^{{\rm o}}_{\rm 2}$- $5f~^3{\rm G}^{{\rm }}_{\rm 3}$ -1.39 -29.869
6155.14 $3p^3~^3{\rm D}^{{\rm o}}_{\rm 3}$- $5f~^3{\rm G}^{{\rm }}_{\rm 4}$ -0.78 -29.869
6237.32 $3p^3~^3{\rm D}^{{\rm o}}_{\rm 1}$- $5f~^3{\rm F}^{{\rm }}_{\rm 2}$ -1.08 -29.869
6243.82 $3p^3~^3{\rm D}^{{\rm o}}_{\rm 2}$- $5f~^3{\rm F}^{{\rm }}_{\rm 3}$ -1.29 -29.869
6244.47 $3p^3~^3{\rm D}^{{\rm o}}_{\rm 2}$- $5f~^1{\rm D}^{{\rm }}_{\rm 2}$ -1.29 -29.869

6347.10
$4s~^2{\rm S}^{{\rm }}_{\rm 1/2}$- $4p~^2{\rm P}^{{\rm o}}_{\rm 3/2}$ 0.26 -30.200
6371.36 $4s~^2{\rm S}^{{\rm }}_{\rm 1/2}$- $4p~^2{\rm P}^{{\rm o}}_{\rm 1/2}$ -0.06 -30.200
* $\log gf$ values have been determined from solar spectrum fits, and damping constants log C6 for Si I lines are computed according to the Anstee & O'Mara (1991, 1995) interpolation tables.

Source LaTeX | All tables | In the text

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