Upper row: maps of Ca ii  H contrast (left) and time-average amplitude of the convective velocity at the bottom photosphere (right). Middle row: power of oscillatory velocity component in the upper photosphere (left) and power of oscillatory component of Ca ii  H intensity (right). Bottom row: map of the magnetic field strength (left) and inclination with respect to the normal to the surface (right) in the observed field of view obtained after inversions of Fe i lines.