Zobrazeno 1 - 10
of 35
pro vyhledávání: '"S. N. Vernov"'
Autor:
V. I. Solovieva, G. V. Kulikov, A.T. Abrosimov, B. A. Khrenov, S. N. Vernov, G. B. Khristiansen, Yu. A. Fomin, N. N. Kalmykov
Publikováno v:
Journal of Physics G: Nuclear Physics. 3:1601-1612
It is shown that, when the scaling in hadron interactions is valid at energies of about 2 x 10'*eV for x = 0.1-1.0 accurate within loo/& the extrapolation of the 'scaling model' to the super-high-energy range 1015-10'7 eV contradicts the experimental
Publikováno v:
Planetary and Space Science. 1:86-93
Measurements made with a scintillation counter installed on the 3rd Soviet earth satellite are presented. By this instrument the counting rate corresponding to the energy greater than 35 keV and the total ionization in the scintillator were measured.
Publikováno v:
Uspekhi Fizicheskih Nauk. 63:149-162
Publikováno v:
AIAA Journal. 1:516-519
Autor:
S. N. Vernov
Publikováno v:
ARS Journal. 31:399-408
Publikováno v:
Uspekhi Fizicheskih Nauk. 63:131-148
Autor:
G. B. Khristiansen, N. N. Kalmykov, O.V. Vedeneev, B. A. Khrenov, S. N. Vernov, Yu. A. Nechin
Publikováno v:
Canadian Journal of Physics. 46:S110-S114
The results of the experimental study of the burst spectrum in ionization chambers underground accompanied by EAS are presented. The investigations were carried out at depths of 20 and 40 m.w.e. The absence of absorption of the burst intensity with i
Publikováno v:
ARS Journal. 31:967-970
T INSTRUMENTATION for measurement of radiation aboard the second Soviet cosmic rocket launched to the moon on Sept. 12, 1959 was installed with the objective of obtaining new data on the outer radiation belt of Earth, recording the radiation of cosmi
Autor:
G. B. Khristiansen, A.T. Abrosimov, G. V. Kulikov, V. B. Atrashkevitch, I. F. Beljaeva, B. A. Khrenov, S. N. Vernov, K.V. Mandritskaya, V. I. Solovjeva
Publikováno v:
Canadian Journal of Physics. 46:S197-S200
Experimental EAS spectra of sizes and muon numbers and results on the fluctuations of the electron–photon and muon EAS components at sea level are presented. In constructing size spectra the sizes of showers were determined by use of the individual
Publikováno v:
Planetary and Space Science. 11:567-574
The third Soviet satellite in an orbit with perigee 187 km, apogee 265 km, and inclination to the equatorial plane of 65 deg , made it possible to trace the variation in the intensity and geographical position of the radiation belts on transition to