Fig. 7

Theoretical Stokes I, V and CSV profiles corresponding to a) the magnetic field map of V410 Tau shown in Fig. 5 and b) the same map scaled by a factor of 10. In each case the CSV column compares obtained from the Stokes I and V line profiles (solid line) with the results of numerical integration of the line-of-sight magnetic field component over the stellar disk (dashed line).
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