Add to ORKGThe energy spectra of high energy gamma-rays and hadrons were obtained by the emulsion chamber with 40 c.u. thickness at Mt. Fuji (3750 m). These results are compared with the Monte Carlo calculation based on the same model which is used in a family analysis. Our data are compatible with the model of heavy-enriched primary and scaling in the fragmentation region
The compilation of ultra high energy jets suggests at present the existence of a bump in primary ene...
Emulsion experiments placed at high mountain altitudes register hadrons and high-energy γ-rays with ...
The characteristics of hadrons of energy > 300 Gev in extensive air showers of size 5.10(^4) - 1.6.1...
Scaling, mean P sub t, high P sub t jets and others at energies over 1000 TeV are discussed on the b...
General features of family events with Summary E sub gamma 200 TeV, observed by the emulsion chambe...
Experimental results from Emulsion Chamber (EC) experiments at mountain altitudes or at higher level...
In order to get higher efficiencies for detecting hadrons and to make technical improvements in the ...
To investigate the chemical composition of primary cosmic rays, several emulsion chambers were expos...
Information on the fragmentation region in super high energy hadronic interactions can be obtained t...
For three different interaction models we have simulated gamma-hadron families, including the detect...
At present the study of nuclear interactions induced by cosmic rays is the unique source of informat...
We show that the simplest assumptions for the dynamics of particle production allow us to understand...
We have observed atmospheric gamma rays from 30GeV to 8TeV, using emulsion chambers at balloon altit...
The lateral distribution of gamma-families observed by emulsion chamber is sensitive to test transve...
A detailed study of the cores of extensive air showers (EAS) at mountain level (Tien-Shan 690 g/cm2)...
The compilation of ultra high energy jets suggests at present the existence of a bump in primary ene...
Emulsion experiments placed at high mountain altitudes register hadrons and high-energy γ-rays with ...
The characteristics of hadrons of energy > 300 Gev in extensive air showers of size 5.10(^4) - 1.6.1...
Scaling, mean P sub t, high P sub t jets and others at energies over 1000 TeV are discussed on the b...
General features of family events with Summary E sub gamma 200 TeV, observed by the emulsion chambe...
Experimental results from Emulsion Chamber (EC) experiments at mountain altitudes or at higher level...
In order to get higher efficiencies for detecting hadrons and to make technical improvements in the ...
To investigate the chemical composition of primary cosmic rays, several emulsion chambers were expos...
Information on the fragmentation region in super high energy hadronic interactions can be obtained t...
For three different interaction models we have simulated gamma-hadron families, including the detect...
At present the study of nuclear interactions induced by cosmic rays is the unique source of informat...
We show that the simplest assumptions for the dynamics of particle production allow us to understand...
We have observed atmospheric gamma rays from 30GeV to 8TeV, using emulsion chambers at balloon altit...
The lateral distribution of gamma-families observed by emulsion chamber is sensitive to test transve...
A detailed study of the cores of extensive air showers (EAS) at mountain level (Tien-Shan 690 g/cm2)...
The compilation of ultra high energy jets suggests at present the existence of a bump in primary ene...
Emulsion experiments placed at high mountain altitudes register hadrons and high-energy γ-rays with ...
The characteristics of hadrons of energy > 300 Gev in extensive air showers of size 5.10(^4) - 1.6.1...