Emission levels in pseudo-continua around the G-band for different magnetic field strengths, relative to the zero-field case at solar disk center, and for different center-to-limb positions. For 800 and 1600 G (80 and 160 mT), the crossover to bright regions (faculae) is seen when moving toward the limb. For the strongest magnetic fields the fluxes become faint, and dark pores begin to form.