Add to ORKGThe energy spectra of atmospheric cosmic rays at Mt. Kanbala (520 g/sq cm.) are measured with emulsion chambers. The power indexes of the spectra are values of about 2.0 for both gamma-rays and hadrons. Those fluxes are consistent with the ones expected from the model of primary cosmic rays with heavy nuclei of high content in the energy around 10 to the 15th power eV
Based on the air shower data, the chemical composition of the primary cosmic rays in the energy rang...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of Yangbajing in Tibet...
We have observed atmospheric gamma rays from 30GeV to 8TeV, using emulsion chambers at balloon altit...
General features of family events with Summary E sub gamma 200 TeV, observed by the emulsion chambe...
In order to get higher efficiencies for detecting hadrons and to make technical improvements in the ...
Experimental results from Emulsion Chamber (EC) experiments at mountain altitudes or at higher level...
Information on the fragmentation region in super high energy hadronic interactions can be obtained t...
The energy spectra of high energy gamma-rays and hadrons were obtained by the emulsion chamber with ...
At present the study of nuclear interactions induced by cosmic rays is the unique source of informat...
The results are presented for the systematic measurement of cosmic ray showers in the first carbon c...
We show that the simplest assumptions for the dynamics of particle production allow us to understand...
A brief review of the energy spectrum of primary cosmic rays above $10^{10}$ eV and the measurement ...
Energy spectra for primary cosmic rays C-Fe above 20 GeV/n were measured on a balloon flight from Gr...
The composition and energy spectra of cosmic rays above 1.6 nJ (10 GeV) on balloons and ultimately o...
A detailed study of the cores of extensive air showers (EAS) at mountain level (Tien-Shan 690 g/cm2)...
Based on the air shower data, the chemical composition of the primary cosmic rays in the energy rang...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of Yangbajing in Tibet...
We have observed atmospheric gamma rays from 30GeV to 8TeV, using emulsion chambers at balloon altit...
General features of family events with Summary E sub gamma 200 TeV, observed by the emulsion chambe...
In order to get higher efficiencies for detecting hadrons and to make technical improvements in the ...
Experimental results from Emulsion Chamber (EC) experiments at mountain altitudes or at higher level...
Information on the fragmentation region in super high energy hadronic interactions can be obtained t...
The energy spectra of high energy gamma-rays and hadrons were obtained by the emulsion chamber with ...
At present the study of nuclear interactions induced by cosmic rays is the unique source of informat...
The results are presented for the systematic measurement of cosmic ray showers in the first carbon c...
We show that the simplest assumptions for the dynamics of particle production allow us to understand...
A brief review of the energy spectrum of primary cosmic rays above $10^{10}$ eV and the measurement ...
Energy spectra for primary cosmic rays C-Fe above 20 GeV/n were measured on a balloon flight from Gr...
The composition and energy spectra of cosmic rays above 1.6 nJ (10 GeV) on balloons and ultimately o...
A detailed study of the cores of extensive air showers (EAS) at mountain level (Tien-Shan 690 g/cm2)...
Based on the air shower data, the chemical composition of the primary cosmic rays in the energy rang...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of Yangbajing in Tibet...
We have observed atmospheric gamma rays from 30GeV to 8TeV, using emulsion chambers at balloon altit...