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The broadband solar K-corona is linearly polarized due to Thomson scattering.Various strategies have been used to represent coronal polarization. Here, wepresent a new way to visualize the polarized corona, using observations fromthe 2023 April 20 total solar eclipse in Australia in support of the CitizenCATE 2024 project. We convert observations in the common four-polarizerorthogonal 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 colorchannels. The unique image generated provides some sense of how humans mightvisualize polarization if we could perceive it in the same way we perceivecolor.

A Chromatic Treatment of Linear Polarization in the Solar Corona at the 2023 Total Solar Eclipse