Radio-Based Study of Characteristics of Cosmic Rays with Highest Energies at Frequency of 30–35 MHz at the Yakutsk Array

2021 ◽  
Vol 85 (8) ◽  
pp. 901-903
Author(s):  
S. P. Knurenko ◽  
I. S. Petrov
Keyword(s):  
Cosmic Rays ◽  
Yakutsk Array

scholarly journals Enhancement of the Yakutsk array by atmospheric Cherenkov telescopes to study cosmic rays above 1015 eV

2010 ◽  
Vol 6 (1) ◽  
pp. 53-57 ◽  
Author(s):  
A. A. Ivanov ◽  
S. P. Knurenko ◽  
Z. E. Petrov ◽  
M. I. Pravdin ◽  
I. Ye. Sleptsov
Keyword(s):  
Cosmic Rays ◽  
Cherenkov Telescopes ◽  
Yakutsk Array

scholarly journals Large-scale distribution of cosmic rays in right ascension as observed by the Yakutsk array at energies above 1018eV

2015 ◽  
Vol 62 ◽  
pp. 1-6 ◽  
Author(s):  
A.A. Ivanov ◽  
A.D. Krasilnikov ◽  
M.I. Pravdin ◽  
A.V. Sabourov
Keyword(s):  
Cosmic Rays ◽  
Large Scale ◽  
Yakutsk Array ◽  
Right Ascension

scholarly journals Upper limit on the fraction of the cosmic ray flux from a separable source in the energy interval (1017 -1019 eV), estimated using data from the Yakutsk array

2019 ◽  
Vol 208 ◽  
pp. 02005
Author(s):  
Anatoly Ivanov
Keyword(s):  
Cosmic Rays ◽  
Cosmic Ray ◽  
High Energy ◽  
Angle Distribution ◽  
Air Showers ◽  
Yakutsk Array ◽  
High Energy Cosmic Rays ◽  
Upper Limit ◽  
Uniform Background ◽  
Using Data

Arrival directions of ultra-high energy cosmic rays (UHECRs) in the equatorial system, detected with the Yakutsk array in the energy range (1017 -10 19 eV), are re-analyzed using a new approximation for the zenith angle distribution of the event rate of extensive air showers (EAS). While the null hypothesis cannot be rejected based on the data used here, an upper limit on the fraction of cosmic rays from a separable source in the uniform background is derived as a function of declination and energy.

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