  The harmonic analysis of anisotropy of Ultra High Energy Cosmic Rays is
performed for the Dark Matter halo model. In this model the relic superheavy
particles comprise part of the Dark Matter and are concentrated in the Galactic
halo. The Ultra High Energy Cosmic Rays are produced by the decays of these
particles. Anisotropy is caused by the non-central position of the Sun in the
Galactic halo. The calculated anisotropy is in reasonable agreement with the
AGASA data. For more precise test of the model a comparison of fluxes in the
directions of the Galactic Center and Anticenter is needed.
