Line profiles and reconstructed brightness and magnetic field distribution of EK Dra. The observed LSD profiles are represented by the black solid lines and the corresponding model profiles are represented by the blue dashed lines. Both the Stokes I and V profiles have been shifted vertically and the Stokes V profiles have been magnified by a factor of 60. Rotational phases are indicated next to each profile. The stellar surface is shown at two different rotational phases. The brightness distribution is shown in the top row of spherical maps; the radial, meridional, and azimuthal field distributions are shown in the following three rows. The magnetic field strength is given in G. The upper set of profiles and maps corresponds to the 2007.1 epoch and the lower to the 2012.1 epoch.