  The correlation between the pointing direction of ultra high energy cosmic
rays and AGN observed by the Pierre Auger Collaboration is explained in the
framework of acceleration process in AGN. This acceleration process is produced
by a rotating accretion disk around a black hole that is frozen-in magnetic
field. In a result the accretion disk is acting as a induction accelerator of
cosmic rays. We estimate the resulting magnetic field in the framework of the
magnetic coupling process. The results of our calculations allow to make the
conclusion that the Flat Spectrum Radio Quasars appear the effective cosmic
accelerators. We estimate also the attenuation of highest-energy cosmic rays in
a result of their interaction with ambient radiation field.
