Fig. 2.

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Intensity (upper panels) and Stokes Q/I (lower panels) profiles as a function of air wavelength, for the 0.8 Å–wide spectral ranges centered on the K I D2 (left panels) and D1 (right panels) lines. Calculations were carried out using the radiative transfer (RT) code introduced in Sect. 2, considering a two-term atomic model with HFS, accounting for partial frequency redistribution (PRD) effects, and in the absence of a magnetic field. For all the figures in this work, a line of sight (LOS) with μ = 0.2 is taken except where otherwise noted. The results of calculations considering the two most abundant isotopes of potassium (solid red curves) are compared to those in which only 39K was considered (solid black curves). The atmospheric model C of Fontenla et al. (1993), hereafter FAL-C, was considered for both calculations. Throughout this work, the reference direction for positive Stokes Q is taken to be parallel to the limb.
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