Fig. C.1
 
      Upper left: plot of the
                       redistribution function defined in Eq. (61), as a function of the reduced frequency of the incoming photons
                  (x′). Each curve corresponds to a
                different (integer) value of the reduced frequency of the outgoing photon
                  (x).
                For some curves, the value of x is indicated in the plot. The reduced
                frequencies x and x′ are
                defined with respect to the frequency ν0 corresponding to the energy
                separation between the centers of gravity of the two terms (x = (ν0 − ν)/ΔνD,
                  x′ = (ν0 − ν′)/ΔνD).
                We consider a 2S − 2P
                transition, the two fine-structure components having a separation of 15 Doppler
                widths (the energies of the upper levels are calculated according to the
                  L − S coupling scheme). We
                assume an Einstein coefficient Auℓ = 108
                  s-1, a
                Doppler width ΔλD = 60 mÅ, and we accordingly
                calculate the damping constant as a = Auℓ/(4πΔνD) ≈ 10-3
                (collisional broadening is neglected, and the conversion of the Doppler width from
                wavelength units to frequency units is made assuming that the transitions fall at
                5000 Å). Upper right: same as upper left, but
                considering only a few values of x (indicated in the plot). Lower
                  left: same as upper left, but for the
                redistribution function defined in Eq. (61), as a function of the reduced frequency of the incoming photons
                  (x′). Each curve corresponds to a
                different (integer) value of the reduced frequency of the outgoing photon
                  (x).
                For some curves, the value of x is indicated in the plot. The reduced
                frequencies x and x′ are
                defined with respect to the frequency ν0 corresponding to the energy
                separation between the centers of gravity of the two terms (x = (ν0 − ν)/ΔνD,
                  x′ = (ν0 − ν′)/ΔνD).
                We consider a 2S − 2P
                transition, the two fine-structure components having a separation of 15 Doppler
                widths (the energies of the upper levels are calculated according to the
                  L − S coupling scheme). We
                assume an Einstein coefficient Auℓ = 108
                  s-1, a
                Doppler width ΔλD = 60 mÅ, and we accordingly
                calculate the damping constant as a = Auℓ/(4πΔνD) ≈ 10-3
                (collisional broadening is neglected, and the conversion of the Doppler width from
                wavelength units to frequency units is made assuming that the transitions fall at
                5000 Å). Upper right: same as upper left, but
                considering only a few values of x (indicated in the plot). Lower
                  left: same as upper left, but for the
                       redistribution function. Lower right: same as lower
                  left, but considering only a few values of x (indicated in the
                plot). The inset panel is a zoom of the line core region of the
                1/2–1/2 transition, showing in more details the curves obtained for values of
                  x
                close to x = 10 (the frequency position of the 1/2–1/2
                transition).
                redistribution function. Lower right: same as lower
                  left, but considering only a few values of x (indicated in the
                plot). The inset panel is a zoom of the line core region of the
                1/2–1/2 transition, showing in more details the curves obtained for values of
                  x
                close to x = 10 (the frequency position of the 1/2–1/2
                transition).
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