Inversions of the Stokes I, Q, U, and V averaged profiles at the location (29′′, 19′′) of the map in Fig. 1. The fits (dashed, dash-dotted, dotted, dash-dot-dotted and long dashed lines) to the observed profiles (solid lines) are obtained by allowing five different atmospheric components to describe the He I triplet. Left a)–d): the dashed profile is obtained by leaving the magnetic field vector free between the five He components while the dash-dotted profile is obtained by coupling only the magnetic field strength. Right e)–h): the dotted profile is obtained by coupling the magnetic field vector between the five He components, coupling the magnetic field strength and the inclination gives the dash-dot-dotted profiles, while coupling the field strength and the azimuth leads to the long dashed profiles.