Physics
Scientist
Characteristics of Hadronic Interactions over 1015eV Observed in High Energy Cosmic-Ray Families in Chacaltaya and Pamir Emulsion Chambers. (I)
Experiment Pamir. I. Energy Spectra of γ -Quanta at the Altitude of 4370 m and 4880 m
Experiment Pamir. II. γ-Families with Energy 30 - 500 TeV
Experiment Pamir. III. Preliminary Data on γ-Quantum and Hadron Families with Energies ΣE > 500 TeV
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