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Fig. 11.

image

UV resonance-line profiles obtained from our 3D code, for the MHD simulation (black, as Fig. 10), and the different ADM models, (i)–(iv) (see text). The line-strength parameter has been set to κ0 = 1. The upper and lower panels show the synthetic profiles for pole-on and equator-on view, respectively. As in Fig. 10, the abscissa has been scaled to v = 2700 km s−1, the “observed” 1D value applied by Marcolino et al. (2013).

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