Azimuthal averages of the magnetic field components (strength, B_tot, inclination, γ, vertical component, B_z, and horizontal component, B_hor) at different distances from the sunspot center are shown. The data are presented for each spectral line in the umbra and penumbra. The x axis represents the distance from the center of the sunspot. The vertical black lines indicate the boundaries between the umbra and the penumbra and between the penumbra and the quiet Sun.