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The initial success of the Rigidly Rotating Magnetosphere (RRM) model application to the B2Vp star σ Ori E by Townsend, Owocki & Groote triggered a renewed era of observational monitoring of this archetypal object. We utilize high-resolution spectropolarimetry and the magnetic Doppler imaging (MDI) technique to simultaneously determine the magnetic configuration, which is predominately dipolar, wi...

Revisiting the rigidly rotating magnetosphere model for σ Ori E – II. Magnetic Doppler imaging, arbitrary field RRM, and light variability★