Fig. 3
SE formation of Hα, Lyα, and Lyβ in the FCHHT-B atmosphere of Fontenla et al. (2009) in the format of Fig. 1, using RH results from Rutten & Uitenbroek (2012). Lefthand panel: NLTE departure coefficients b for hydrogen levels n = 1,2,3. The dashed and dotted NLTE and LTE fractional population curves are for n = 2. Righthand panel: corresponding line source functions.
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