Alpha particle and proton fluxes of the primary cosmic radiation and their time variations

1962 ◽  
Vol 24 (9) ◽  
pp. 779-784 ◽  
Author(s):  
E. Waibel
Keyword(s):  
Alpha Particle ◽  
Cosmic Radiation ◽  
Proton Fluxes ◽  
Primary Cosmic Radiation ◽  
Time Variations

scholarly journals The search of the anisotropy of the primary cosmic radiation by the difference method

2017 ◽  
Vol 145 ◽  
pp. 03003
Author(s):  
Victor Pavlyuchenko ◽  
Romen Martirosov ◽  
Natalia Nikolskaya ◽  
Anatoly Erlykin
Keyword(s):  
Difference Method ◽  
Cosmic Radiation ◽  
Primary Cosmic Radiation ◽  
The Difference

The Determination of the Sign and the Energy Spectrum of Primary Cosmic Radiation

1947 ◽  
Vol 71 (7) ◽  
pp. 393-398 ◽  
Author(s):  
M. S. Vallarta ◽  
M. L. Perusquía ◽  
J. de Oyarzábal
Keyword(s):  
Energy Spectrum ◽  
Cosmic Radiation ◽  
Primary Cosmic Radiation

The Detection of Heavy Particles in the Primary Cosmic Radiation

1949 ◽  
Vol 76 (7) ◽  
pp. 997-998 ◽  
Author(s):  
Martin A. Pomerantz ◽  
Frank L. Hereford
Keyword(s):  
Cosmic Radiation ◽  
Heavy Particles ◽  
Primary Cosmic Radiation

scholarly journals INFLUENCE OF PRIMARY COSMIC RADIATION MASS COMPOSITION ON THE ESTIMATION OF EAS ENERGY

2005 ◽  
Vol 20 (29) ◽  
pp. 6897-6899 ◽  
Author(s):  
S. P. KNURENKO ◽  
A. A. IVANOV ◽  
V. A. KOLOSOV ◽  
Z. E. PETROV ◽  
I. YE. SLEPTSOV ◽  
...  
Keyword(s):  
Cosmic Radiation ◽  
Cherenkov Radiation ◽  
Charged Particles ◽  
Mass Composition ◽  
Mixed Composition ◽  
Radiation Data ◽  
Primary Particles ◽  
Primary Cosmic Radiation ◽  
Electron Photon ◽  
Photon Component

Fraction of energy, E em /E0, transferred to the electron-photon component of EAS at E0 = 1015 ± 1019 eV was estimated by using the Cherenkov radiation data and the data on charged particles obtained at the Yakutsk EAS array. The results are compared with predictions of different models for energy dissipation into the EAS electron-photon component and with calculations performed with different primary nuclei content. In the energy ranges 1015 ± 1016 eV and 1018 ± 1019 eV , the ratio E em /E0 is equal to (77 ± 2)% and (88 ± 2)%, respectively, that does not contradict to a mixed composition of primary particles in the first energy interval and purely proton composition in the second one.

The HERO project for the study of high-energy primary cosmic radiation

2009 ◽  
Vol 73 (5) ◽  
pp. 593-596
Author(s):  
D. M. Podorozhnyi ◽  
E. V. Atkin ◽  
L. S. Burylov ◽  
A. G. Voronin ◽  
N. V. Kuznetsov ◽  
...  
Keyword(s):  
Cosmic Radiation ◽  
High Energy ◽  
Primary Cosmic Radiation
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