We present all-particle primary cosmic-ray energy spectrum in the 3-200 PeV energy range obtained by a multi-parametric event-by-event evaluation of the primary energy. The results are obtained on the basis of an expanded EAS dataset detected at mountain level (700 g/cm^2) by the GAMMA experiment. The energy evaluation method has been developed using the EAS simulation with the SIBYLL interaction model taking into account the response of GAMMA detectors and reconstruction uncertainties of EAS parameters. Nearly unbiased (<5%) energy estimations regardless of a primary nuclear mass with an accuracy of about 15-10% in the 3-200 PeV energy range respectively are attained. An irregularity ('bump') in the spectrum is observed at primary energies...
Multimuon data from the MACRO experiment at Gran Sasso have been analyzed using a new method, which ...
Cosmic ray in the 1015–1018 eV energy range can only be detected with ground based experiments, samp...
Multimuon data from the MACRO experiment at Gran Sasso have been analyzed using a new method, which ...
International audienceWe present all-particle primary cosmic-ray energy spectrum in the 3-200 PeV en...
"We present an all-particle primary cosmic-ray energy spectrum in the 3 x 106-2 x 108 GeV energy ran...
Proceedings of the XIV International Symposium on Very High Energy Cosmic Ray InteractionsInternatio...
[著者版]We present an updated all-particle energy spectrum of primary cosmic rays in a wide range from ...
11 pages, 14 figures, submitted to 29th International Cosmic Ray Conference, PuneOn the basis of the...
On the basis of the extensive air shower (EAS) data obtained by the GAMMA experiment, the energy spe...
The energy spectrum of primary cosmic rays in the energy range of 10 eV is infered from the inf...
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...
The break observed in the electron shower size power law spectrum of Extensive Air Showers (EAS) at ...
The energy spectrum of cosmic rays with primary energies between 1014 eV and 1016 eV has been studie...
Muon-electron ratio and median zenith angle of Extensive Air Shower (EAS) is calculated for the ener...
Multimuon data from the MACRO experiment at Gran Sasso have been analyzed using a new method, which ...
Cosmic ray in the 1015–1018 eV energy range can only be detected with ground based experiments, samp...
Multimuon data from the MACRO experiment at Gran Sasso have been analyzed using a new method, which ...
International audienceWe present all-particle primary cosmic-ray energy spectrum in the 3-200 PeV en...
"We present an all-particle primary cosmic-ray energy spectrum in the 3 x 106-2 x 108 GeV energy ran...
Proceedings of the XIV International Symposium on Very High Energy Cosmic Ray InteractionsInternatio...
[著者版]We present an updated all-particle energy spectrum of primary cosmic rays in a wide range from ...
11 pages, 14 figures, submitted to 29th International Cosmic Ray Conference, PuneOn the basis of the...
On the basis of the extensive air shower (EAS) data obtained by the GAMMA experiment, the energy spe...
The energy spectrum of primary cosmic rays in the energy range of 10 eV is infered from the inf...
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...
The break observed in the electron shower size power law spectrum of Extensive Air Showers (EAS) at ...
The energy spectrum of cosmic rays with primary energies between 1014 eV and 1016 eV has been studie...
Muon-electron ratio and median zenith angle of Extensive Air Shower (EAS) is calculated for the ener...
Multimuon data from the MACRO experiment at Gran Sasso have been analyzed using a new method, which ...
Cosmic ray in the 1015–1018 eV energy range can only be detected with ground based experiments, samp...
Multimuon data from the MACRO experiment at Gran Sasso have been analyzed using a new method, which ...