Results of the two-component inversions of the He I lines for AR 12552 observed on 09 June 2016 (data set 8). Panels a–c: normalized intensity at 10 825 Å, the normalized intensity at the He Ic line center, and the Stokes V/I_c signal at 10 826.89 Å, respectively. The LOS velocity, the magnetic field strength, and the LOS inclination of the magnetic field are presented in panels d–f for the slow component and in panels g–i for the supersonic component. The contours mark the boundaries of sunspots and pores, determined using the continuum intensity image shown in panel a. These contours enclose regions within the 85% level of the surrounding quiet Sun intensity in the continuum image. The arrows in panel a indicate solar north and east. The azimuths of the magnetic field are overplotted as lines in panels d and g. See Sect. 3 for further details.