  The broadband solar K-corona is linearly polarized due to Thomson scattering.
Various strategies have been used to represent coronal polarization. Here, we
present a new way to visualize the polarized corona, using observations from
the 2023 April 20 total solar eclipse in Australia in support of the Citizen
CATE 2024 project. We convert observations in the common four-polarizer
orthogonal basis (0{\deg}, 45{\deg}, 90{\deg}, & 135{\deg}) to -60{\deg},
0{\deg}, and +60{\deg} (MZP) polarization, which is homologous to R, G, B color
channels. The unique image generated provides some sense of how humans might
visualize polarization if we could perceive it in the same way we perceive
color.
