  Simultaneously and coherently studying the large-scale magnetic field and the
stellar pulsations of a massive star provides strong complementary diagnostics
suitable for detailed stellar modelling. This hybrid method is called
magneto-asteroseismology and permits the determination of the internal
structure and conditions within magnetic massive pulsators, for example the
effect of magnetism on non-standard mixing processes. Here, we overview this
technique, its requirements, and list the currently known suitable stars to
apply the method.
