Physics
Scientist
ANK, Inst. Fiziki Vysokikh Ehnergij, Alma-Ata, Kazakhstan
Characteristics of anomalously high multiplicity cosmic ray interactions
Comparison of Experimental and Calculated Characteristic of Gamma-Quanta Families at Σ Eγ ≳ 5 Tev
Comparison of hadron chamber data from the PAMIR experiment with model calculations for different chemical compositions of primary cosmic rays
High Energy Gamma-Quanta in Hadron-Nuclear Interactions at Primary Energies Exceeding 2. 5 TeV
Installation for Big Multiplicity Interactions Registration
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