PF observation 34 (upper panel) and PF observation one (lower panel) showing the areas of high probability in comparison with the continuum, the magnetogram, and the AIA 304 channel of SDO. In the upper panel the area of high probability flagged by our models spans the entire area of increased magnetic field but also extends beyond the edges of the penumbra. In the lower panel we also see how the area of high importance spans over the areas of strong magnetic fields but additionally covers the area in between, where the photospheric magnetic field is weak.