Physics
Scientist
"pamir" Experiment Iii: Partial Inelasticity Coefficient at Hadron Energies of 10**13 - 10**14 EV
Calculation of Characteristics of Gamma-Families with E >= 500 Tev II. Characteristics of Gamma-Ray Superfamilies Without Halo, Realistic Model of Hadron Interaction at Energies >=10**15 EV
Calculation of Characteristics of Gamma-Families with Σ Eγ>= 500 Tev I. Characteristics of Interaction Models, Testing by Calculational Results, Gamma-Families with Halo with ΣEγ>=500 Tev
Characteristics of Hadronic Interactions over 1015eV Observed in High Energy Cosmic-Ray Families in Chacaltaya and Pamir Emulsion Chambers. (I)
Experiment " PAMIR " IV : the Fraction of Single High Energy Hadrons and Inelasticity Coefficient at Energies 10**15 - 10**16 EV
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