Solar Corona Polarization and Neutrino Behavior via AF Model

We investigated the predictive power of the Actualization Function (AF) model for polarization structures and neutrino fluxes in the solar corona. By normalizing AF predictions to real measured data, we confirmed excellent numeric shape alignment for polarization profiles. Conversely, numeric tests of AF predictions for neutrino emission found no measurable correlation, indicating negligible AF contribution to solar neutrino flux.