  We study anisotropy of cosmic rays in the energy range 0.2-1.4 EeV at
intermediate angular scales using the public data set of the Pierre Auger
Observatory. At certain scales, the analysis reveals a number of deviations
from the isotropic distribution with the statistical significance above three
standard deviations. It also demonstrates that the anisotropy evolves with
energy. If confirmed with the complete Auger or Telescope Array data sets, the
result can shed new light on the structure of galactic magnetic fields and the
problem of transition from galactic to extragalactic cosmic rays.
