  Zeeman Doppler Imaging is a powerful tool for characterizing the strength and
topology of stellar magnetic fields. In this research note, we present a new
way to visualize the typical results from ZDI for an ensemble of stars,
addressing some of the concerns with the standard `confusogram' approach to
illustrating the data. Our publically available plotting methods further enable
an accessible means to consider variability in the inferred magnetic field
topologies from repeated observations, as we demonstrate with the literature
ZDI data on M dwarfs.
