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Fig. 7.


Similar to Fig. 5 for the different field strength cases in Beeck et al. (2013). The “500 H” case used the “500 G” simulation but with the field set to zero in the radiative transfer calculations. All cases are for the G2 star using the 6173 Å line, no rotation, i = 0° and m = 0 and the visibilities have been divided by the one for m = l = 0.

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