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Publications in Math-Net.Ru
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What should be the spectrum of galactic cosmic rays?
Pis'ma v Zh. Èksper. Teoret. Fiz., 74:3 (2001), 147–150
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The share of protons in cosmic ray flux at the energies $\gtrsim25$ TeV
Dokl. Akad. Nauk SSSR, 308:4 (1989), 850–853
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Radioactive nuclei as a possible source of the electrons with the energy of $10$–$100$ Mev in the Earth radiation belt inner zone
Dokl. Akad. Nauk SSSR, 295:3 (1987), 583–586
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Electrons with energy $E>100$ Mev, captured by the Earth magnetic field
Dokl. Akad. Nauk SSSR, 282:1 (1985), 81–83
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Development of the ionization calorimeter method applied to the problem of small intensity
cosmic ray isotonic composition study
Dokl. Akad. Nauk SSSR, 264:2 (1982), 334–338
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On the possibility of existence of the Earth radiation belt consisting of electrons with energies of 100 Mev and higher
Dokl. Akad. Nauk SSSR, 234:4 (1977), 810–813
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On collective interactions of nucleons of high-energy cosmic ray heavy nuclei
Dokl. Akad. Nauk SSSR, 202:1 (1972), 65–66
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Investigation of the soft corpuscular radiation at the Luna-10 satellite of the Moon
Dokl. Akad. Nauk SSSR, 170:3 (1966), 567–569
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Investigation of the cosmic radiation at Luna-10 satellite
Dokl. Akad. Nauk SSSR, 170:3 (1966), 565–566
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Measurement of cosmic radiation on the sputnik
Dokl. Akad. Nauk SSSR, 120:6 (1958), 1231–1233
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Cross-section for inelastic proton-proton interaction at proton energies greater than 7 Bev
Dokl. Akad. Nauk SSSR, 117:4 (1957), 593–596
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The cross-section for inelastic interaction of more than 7 Bev kinetic energy protons with nuclei of carbon atoms
Dokl. Akad. Nauk SSSR, 115:2 (1957), 259–262
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Determination of the flux of primary cosmic ray particles at $31^\circ$ $\mathrm{N}$ latitude
Dokl. Akad. Nauk SSSR, 115:1 (1957), 71–74
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Средние характеристики акта взаимодействия первичных космических частиц разных энергий (2–1000 Бэв) с лёгкими атомными ядрами
UFN, 58:4 (1956), 599–666
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Sergei Nikolaevich Vernov (on his seventieth birthday)
UFN, 131:3 (1980), 521–523
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Sergei Nikolaevich Vernov (on his fiftieth birthday)
UFN, 72:1 (1960), 153–155
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