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The study of the evolution of the amplitude and phase of the cosmic ray anisotropy into the energy region 1014 ? 1016 eV can provide a significant tool for the understanding of the knee of the primary spectrum. We extend here the EAS-TOP measurement performed at E0 ~ 1014 eV, to higher energies by using the full data set (8 years). Results derived at about 1014 and 4 ? 1014 eV are compared and discussed. Hints of increasing amplitude and change of phase above 1014 eV are reported.

Evolution of the cosmic ray anisotropy above 1014eV