The amplitude and phase of the cosmic ray anisotropy are well established experimentally between 10(11) eV and 10(14) eV. The study of their evolution into the energy region 10(14) − 10(16) eV can provide a significant tool for the understanding of the steepening (“knee”) of the primary spectrum. In this letter we extend the EAS-TOP measurement performed at E0 ≈ 10(14) eV, to higher energies by using the full data set (8 years of data taking). Results derived at about 10(14) and 4 · 10(14) eV are compared and discussed. Hints of increasing amplitude and change of phase above 10(14) eV are reported. The significance of the observation for the understanding of cosmic ray propagation is discussed
We report a measurement of the energy spectrum of cosmic rays for energies above 2.5×1018 eV based ...
We report a measurement of the energy spectrum of cosmic rays for energies above 2.5×1018 eV based o...
A measurement of the cosmic-ray spectrum for energies exceeding 4x10(18) eV is presented, which ...
The amplitude and phase of the cosmic ray anisotropy are well established experimentally between 10(...
The amplitude and phase of the cosmic-ray anisotropy are well established experimentally between 101...
The study of the evolution of the amplitude and phase of the cosmic ray anisotropy into the energy r...
The cosmic ray energy spectrum in the range E-o = 10(15)-10(16) eV (including the region of the stee...
The cosmic ray energy spectrum in the range E0 = 101511016 eV (including the region of the steepenin...
International audienceWe report a measurement of the energy spectrum of cosmic rays for energies abo...
The results of the measurement of the cosmic-ray solar and sidereal anisotropies at primary energy E...
A survey is made of the anisotropy of cosmic rays at energies above 10 to the 14th power eV. It is c...
We report a measurement of the energy spectrum of cosmic rays for energies above 2.5×1018 eV based ...
We report a measurement of the energy spectrum of cosmic rays for energies above 2.5×1018 eV based o...
A measurement of the cosmic-ray spectrum for energies exceeding 4x10(18) eV is presented, which ...
The amplitude and phase of the cosmic ray anisotropy are well established experimentally between 10(...
The amplitude and phase of the cosmic-ray anisotropy are well established experimentally between 101...
The study of the evolution of the amplitude and phase of the cosmic ray anisotropy into the energy r...
The cosmic ray energy spectrum in the range E-o = 10(15)-10(16) eV (including the region of the stee...
The cosmic ray energy spectrum in the range E0 = 101511016 eV (including the region of the steepenin...
International audienceWe report a measurement of the energy spectrum of cosmic rays for energies abo...
The results of the measurement of the cosmic-ray solar and sidereal anisotropies at primary energy E...
A survey is made of the anisotropy of cosmic rays at energies above 10 to the 14th power eV. It is c...
We report a measurement of the energy spectrum of cosmic rays for energies above 2.5×1018 eV based ...
We report a measurement of the energy spectrum of cosmic rays for energies above 2.5×1018 eV based o...
A measurement of the cosmic-ray spectrum for energies exceeding 4x10(18) eV is presented, which ...