CoMP inversions of the vector coronal magnetic field on 2016 October 14. Top-row panels present one of the four degenerate solutions. Due to the degeneracies in the sign of B_x and B_z that govern each pixel individually, a noise pattern appears in this distinct solution realization. Qualitative ICM-selected realization using the four degenerate solutions are presented in the middle row. PFSS field lines derived from photospheric magnetograms are overplotted. The bottom row presents total magnetic field strength, along with LOS and POS magnitudes in a wider-context FOV.