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Fraction of hot stars posses strong magnetic fields that channel theirradiatively driven outflows. We study the influence of line splitting in themagnetic field (Zeeman effect) on the wind properties. We use our own globalwind code with radiative transfer in the comoving frame to understand theinfluence of the Zeeman splitting on the line force. We show that the Zeemansplitting has a negligible influence on the line force for magnetic fields thatare weaker than about 100~kG. This means that the wind mass-loss rates andterminal velocities are not affected by the magnetic line splitting formagnetic fields as are typically found on the surface of nondegenerate stars.Neither have we found any strong flux variability that would be due to themagnetically split line blanketing.

Hot-star wind models with magnetically split line blanketing