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Magnetic B-type stars exhibit photometric variability due to diverse causes,and consequently on a variety of timescales. In this paper we describeinterpretation of BRITE photometry and related ground-based observations of 4magnetic B-type systems: $\epsilon$ Lupi, $\tau$ Sco, a Cen and $\epsilon$ CMa.

Magnetic B stars observed with BRITE: Spots, magnetospheres, binarity, and pulsations