Fig. 14.

Blue profiles: observations of the Fe I 15648.52 Å (air wavelength) line in the quiet sun (courtesy of Dr. J.M. Borrero; see Kiess et al. 2018). Red profiles: NLTE synthesis obtained with our model assuming a two-level atom for the transition , with Auℓ = 1.94 × 10−6, effective Landé factor
, negligible damping constant a = 0, T = 8000 K, and
. The magnetic field and the LOS are vertical. For obtaining profile 1 (left panel): BLOS = 500 G, Tν0 = 1.0, vLOS = −6.3 km s−1,
,
, rc = 12 (ratio continuum to line opacity). For the profile 2 (right panel): BLOS = 1100 G, Tν0 = 0.35, vLOS = −3.2 km s−1, Scont/Sline = 1.37,
, rc = 18. The I0 was obtained by using the shape of the observed I as seed profile and scaling it with
and
to reproduce simultaneously the observed intensity and Stokes V profiles within a tolerance of 5% of the continuum intensity.
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