  Arrival directions of ultra-high energy cosmic rays from the direction of ten
brightest radio sources lying within 50 Mpc from our Galaxy were studied by
using recent models of the largescale Galactic magnetic field. A detailed
study, where also small-scale turbulent magnetic field component was
implemented, is presented for the radiogalaxy Virgo A. This radiogalaxy is
located far from the Galactic plane which leads to a unique image of this UHECR
source candidate, if the flux is composed from a mixture of intermediate mass
nuclei. We present a method suitable for identifying cosmic rays arriving from
this close-by radiogalaxy.
