Cosmic ray spectrum by energy scattered by EAS particles in the atmosphere and galactic model

Knurenko, S.P.; Ivanov, A.A.; Sabourov, A.V.

doi:10.1134/S0021364007220018

Cosmic ray spectrum by energy scattered by EAS particles in the atmosphere and galactic model

Nov, 2007

7 pages

Published in:

JETP Lett. 86 (2007) 621-624

e-Print:

0711.2548 [astro-ph]

DOI:

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Abstract: (arXiv)

The differential energy spectrum of cosmic rays from Cherenkov radiation measurements in EAS in the energy range of 10^15-10^20eV has been compared with an anomalous diffusion model for the particles in interstellar space having fractal properties (Lagutin et al, 2001). The close association between experimental data and calculated "all particle" spectra in form at E(0) (10^15-10^18)eV is found. In this case, the average mass composition of cosmic rays calculated by five components does not contradict the average mass composition from experimental data which was obtained by several of EAS characteristics in that energy region.

Note:

7 pages, 4 figures

13.85.Tp
13.40.-f
p: cosmic radiation
nucleus: cosmic radiation
showers: air
radiation: Cherenkov
cosmic radiation: energy spectrum
cosmic radiation: mass
diffusion: model
atmosphere

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Cosmic ray spectrum by energy scattered by EAS particles in the atmosphere and galactic model

Citations per year

End to the cosmic ray spectrum?

Upper limit of the spectrum of cosmic rays

The energy spectrum of cosmic rays above 10^15 ev as derived from air Cherenkov light measurements in yakutsk

The knee in the primary cosmic ray spectrum as consequence of the anomalous diffusion of the particles in the fractal interstellar medium

Characteristics of EAS and primary particle mass composition in the energy region of 10**17 - 3 x 10**19 eV by Yakutsk data

Characteristics of EAS and primary particle mass composition in the energy region of 1017 - 3 x 1019 eV by Yakutsk data