EVOLUTION OF THE COSMIC-RAY ANISOTROPY ABOVE 10 <sup>14</sup> eV
EVOLUTION OF THE COSMIC-RAY ANISOTROPY ABOVE 10 <sup>14</sup> eV
The amplitude and phase of the cosmic-ray anisotropy are well established experimentally between 1011 eV and 1014 eV. The study of their evolution in the energy region 1014–1016 eV can provide a significant tool for the understanding of the steepening ("knee") of the primary spectrum. In this Letter, we extend …