Intensity and polarization maps normalized to the continuum intensity of the quiet Sun, I_QS. They show a bipolar region observed with CRISP in the Mg I b₂ 5173 Å line at 07:20 UT. Left: Intensity maps at different wavelengths. Right: Maps of Q and U averaged over three wavelengths in the blue wing (Δλ = −100, −50, and 0 mÅ), and a Stokes V magnetogram at ±50 mÅ from the core. The black arrow points toward the disk center. The red contours in the right panels delineate the boundaries of the pores.