scholarly journals Results of the Further Analysis of Data from the Tien Shan Array in the Energy Spectrum of Primary Cosmic Rays in the Energy Range of $${2\times 10^{13}{-}3\times 10^{17}}$$ eV

2020 ◽  
Vol 83 (4) ◽  
pp. 629-633
Author(s):  
E. N. Gudkova ◽  
N. M. Nesterova
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
Energy Range ◽  
Tien Shan ◽  
Primary Cosmic Rays

scholarly journals Investigation of the energy spectrum and chemical composition of primary cosmic rays in 1–100 PeV energy range with a UAV-borne detector

2020 ◽  
Vol 15 (09) ◽  
pp. C09061-C09061
Author(s):  
D. Chernov ◽  
E. Bonvech ◽  
M. Finger Jr. ◽  
M. Finger ◽  
V. Galkin ◽  
...  
Keyword(s):  
Chemical Composition ◽  
Energy Spectrum ◽  
Cosmic Rays ◽  
Energy Range ◽  
Primary Cosmic Rays

Energy spectrum of primary cosmic rays at energies of 2 × 1013 to 5 × 1017 eV, according to Tien Shan data

2017 ◽  
Vol 81 (4) ◽  
pp. 457-459 ◽  
Author(s):  
E. N. Gudkova ◽  
N. M. Nesterova ◽  
N. M. Nikolskaya ◽  
V. P. Pavlyuchenko
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
Tien Shan ◽  
Primary Cosmic Rays

The study of primary cosmic rays energy spectrum and mass composition in the energy range 0.5 – 50 PeV with TUNKA Eas Cherenkov array

1999 ◽  
Vol 75 (1-2) ◽  
pp. 299-301 ◽  
Author(s):  
O.A. Gress ◽  
T.I. Gress ◽  
E.E. Korosteleva ◽  
L.A. Kuzmichev ◽  
B.K. Lubsandorzhiev ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
Energy Range ◽  
Mass Composition ◽  
Primary Cosmic Rays

Electron component in primary cosmic rays. I. Experiment

1968 ◽  
Vol 46 (10) ◽  
pp. S530-S532 ◽  
Author(s):  
A. Danjo ◽  
S. Hayakawa ◽  
F. Makino ◽  
Y. Tanaka
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
Energy Range ◽  
Power Law ◽  
Differential Spectrum ◽  
Cutoff Rigidity ◽  
Electron Component ◽  
Geomagnetic Cutoff Rigidity ◽  
Geomagnetic Cutoff ◽  
Primary Cosmic Rays

The energy spectrum of electrons in the primary cosmic rays was measured at a location where the vertical geomagnetic cutoff rigidity is 11.5 GV, using a balloon-borne counter system. The differential spectrum was determined in the energy range from 13 to 50 GeV and is represented by a power law with exponent −2.4 ± 0.6. This result is consistent with a spectrum extending smoothly from lower energies with the same slope.

Search for sources of primary cosmic rays at energy above 0.1 PeV at the Tien Shan

2008 ◽  
Vol 175-176 ◽  
pp. 541-543 ◽  
Author(s):  
G. Benkó ◽  
A.P. Chubenko ◽  
G. Erdös ◽  
S.I. Nikolsky ◽  
N.M. Nesterova ◽  
...  
Keyword(s):  
Cosmic Rays ◽  
Tien Shan ◽  
Primary Cosmic Rays

Energy Spectrum of Primary Cosmic Rays, According to TUNKA-133 and TAIGA-HiSCORE EAS Cherenkov Light Data

2019 ◽  
Vol 83 (8) ◽  
pp. 1016-1019 ◽  
Author(s):  
V. V. Prosin ◽  
I. I. Astapov ◽  
P. A. Bezyazeekov ◽  
V. Boreyko ◽  
A. N. Borodin ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
Cherenkov Light ◽  
Primary Cosmic Rays

Integral energy spectrum of primary cosmic rays at high energies

Pramana ◽  
1982 ◽  
Vol 19 (2) ◽  
pp. 133-140
Author(s):  
R Hasan ◽  
S C Arora ◽  
D Hans ◽  
M S Swami
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
High Energies ◽  
Integral Energy ◽  
Integral Energy Spectrum ◽  
Primary Cosmic Rays
Sign in / Sign up

Export Citation Format

Share Document