Inverted maps from STiC at log τ_c = 0.0, representative of the photosphere. From left to right: Vertical magnetic field strength, inclination, azimuth, LOS velocity, v_LOS component, and temperature. The black contours indicate the size of the umbra, and the red contours mark the extent of the penumbra. The vertical dashed lines indicate where we made vertical cuts to analyze the vertical structure of the solar atmosphere. The magnetic field results are transformed to LRF.