  We considered propagation of Ultra High Energy Cosmic Rays (UHECR) through
the galaxy. We investigated models with sources of UHECR distributed in the
same way as Cold Dark Matter (CDM) in a self-consistent way, taking into
account both extra-galactic and Galactic contributions. Using a very simple toy
model of galactic magnetic field we showed that in the case of galactic origin
of UHECRs the anisotropy can reach considerable values. In the case of
extragalactic UHECRs origin the anisotropy appears to be non-vanishing only for
electron and photon components due to synchrotron losses, but it hardly can be
reassured. The reason is an extremely low flux of UHE electrons and a too low
level of gamma-ray anisotropy.
