Table 2
Excerpt from the list of atomic line parameters of the elements used in the analysis and EWs measured in the degraded spectrum of the Solar Flux Atlas.
| λ [Å] | Id. | χ [eV] | log gf | EW [mÅ] |
|
|
||||
| 5247.06 | Fe i | 0.09 | −5.022 | 64.0 |
| 5322.05 | Fe i | 2.28 | −2.878 | 62.6 |
| 5501.48 | Fe i | 0.96 | −3.105 | 121.2 |
| 5522.45 | Fe i | 4.21 | −1.397 | 46.1 |
| 5543.94 | Fe i | 4.22 | −1.055 | 64.7 |
| 5546.51 | Fe i | 4.37 | −1.098 | 54.6 |
| 5560.22 | Fe i | 4.43 | −1.080 | 52.8 |
| 5587.58 | Fe i | 4.14 | −1.738 | 32.0 |
| 5618.64 | Fe i | 4.21 | −1.310 | 50.9 |
| 5619.60 | Fe i | 4.39 | −1.422 | 36.2 |
| ... | ... | ... | ... | ... |
Notes. Lines with missing gf values represent the elements for which the hyperfine structure was taken into account (Mg, V, Mn, and Cu) and the detailed line splitting is shown in Table 3. The whole table is available in electronic form at the CDS.
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