Examples of different structures and their associated Stokes V classes and physical properties. From left to right: eud classification of Mg Stokes V, Fe continuum intensity (at +532 mÅ) normalized to its mean QS value, Mg continuum intensity (at −700 mÅ) normalized to its mean QS value, photospheric LOS velocity from the SIR inversions of the Fe line, Doppler velocity of the Mg line core, unsigned LOS magnetic field from the SIR inversions and from the WFA in the Mg ±100 mÅ spectral window, the photospheric to chromospheric |B_LOS| ratio, and the amplitude asymmetries of the Mg Stokes V profiles. All the examples show a ∼6″ × 6″ sub-field. For each row, the contours enclose the V class specified in the intensity maps.