On the basis of the extensive air shower (EAS) data obtained by the GAMMA experiment, the energy spectra and elemental composition of the primary cosmic rays are derived in the 1 - 100 PeV energy range. The reconstruction of the primary energy spectra is carried out using an EAS inverse approach with the hypothesis of power-law primary energy spectra with rigidity-dependent knees. The rigidity- dependent knee feature of the primary energy spectra is displayed at the rigidities ER similar or equal to 2.5 +/- 0.2 PeV/Z and ER similar or equal to 3.1 - 4.2 PeV/Z for the SIBYLL and QGSJET interaction models respectively.;Using the event-by-event method of the primary energy evaluation from the measured N-ch, N-mu and shower age (s) parameters, ...
A study of the primary cosmic ray composition in the energy range 5.10(14)-5.10(15) eV is performed ...
A study of the primary cosmic ray composition in the energy range 5.10(14)-5.10(15) eV is performed ...
A study of the primary cosmic ray composition in the energy range 5s1014-5s1015 eV is performed thro...
On the basis of the extensive air shower (EAS) data obtained by the GAMMA experiment, the energy spe...
On the basis of the extensive air shower (EAS) data obtained by the GAMMA experiment, the energy spe...
11 pages, 14 figures, submitted to 29th International Cosmic Ray Conference, PuneOn the basis of the...
The evolution of the cosmic ray primary composition in the energy range 10(6)–10(7) GeV (i.e. the ‘‘...
Primary cosmic ray particles above energies of about 100 TeV are investigated by large-area ground b...
In this contribution I will summarize and discuss some recent results about the study of the knee of...
The cosmic ray primary composition in the energy range between 10(15) and 10(16) eV, i.e., around th...
The number of hadrons and their energy sum in extensive air showers has been measured using the KASC...
We present all-particle primary cosmic-ray energy spectrum in the 3-200 PeV energy range obtained by...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the ``...
A study of the primary cosmic ray composition in the energy range 5.10(14)-5.10(15) eV is performed ...
A study of the primary cosmic ray composition in the energy range 5.10(14)-5.10(15) eV is performed ...
A study of the primary cosmic ray composition in the energy range 5s1014-5s1015 eV is performed thro...
On the basis of the extensive air shower (EAS) data obtained by the GAMMA experiment, the energy spe...
On the basis of the extensive air shower (EAS) data obtained by the GAMMA experiment, the energy spe...
11 pages, 14 figures, submitted to 29th International Cosmic Ray Conference, PuneOn the basis of the...
The evolution of the cosmic ray primary composition in the energy range 10(6)–10(7) GeV (i.e. the ‘‘...
Primary cosmic ray particles above energies of about 100 TeV are investigated by large-area ground b...
In this contribution I will summarize and discuss some recent results about the study of the knee of...
The cosmic ray primary composition in the energy range between 10(15) and 10(16) eV, i.e., around th...
The number of hadrons and their energy sum in extensive air showers has been measured using the KASC...
We present all-particle primary cosmic-ray energy spectrum in the 3-200 PeV energy range obtained by...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the ``...
A study of the primary cosmic ray composition in the energy range 5.10(14)-5.10(15) eV is performed ...
A study of the primary cosmic ray composition in the energy range 5.10(14)-5.10(15) eV is performed ...
A study of the primary cosmic ray composition in the energy range 5s1014-5s1015 eV is performed thro...