Table 1: Spectral lines used in this study. Lines are given depending on their forming region: from the upper part to the lower part of the atmosphere. Line-forming regions have been determined using the hydrodynamical model defined by $\tau _{\rm l}=2/3$ where $\tau _{\rm l}$ is the optical depth at the centre of the line (see Fig. 8). The line depth (in percentage of the continuum) is indicated.

Name

Wavelength (Å) Line depth
    (% of the continuum)

Fe I

6003.012 18
Fe I 6056.005 16
Fe I 6380.743 9
Ni I 6378.247 5

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