The energy spectrum of primary cosmic rays with ultra high energies based on the Yakutsk EAS Array data is presented. For the largest events values of S600 and axis coordinates have been obtained using revised lateral distribution function. The affect of the arrival time distribution at several axis distance on estimated density for Yakutsk and AGASA is considered
The break observed in the electron shower size power law spectrum of Extensive Air Showers (EAS) at ...
[著者版]We present an updated all-particle energy spectrum of primary cosmic rays in a wide range from ...
International audienceThe two-point autocorrelation function of ultra-high energy cosmic ray (UHECR)...
In this work the energy spectrum of cosmic rays based on Yakutsk EAS array data is presented. After ...
The experimental data on the cosmic ray energy spectrum obtained from the Small Cherenkov Array in Y...
The Yakutsk array observes the Cherenkov light emitted by UHECR in atmosphere. Recently, an autonomo...
The experimental data on the cosmic ray energy spectrum obtained from the Small Cherenkov Array in Y...
A spectrum of cosmic rays within energy range 1015 − 3 × 1017 eV was derived from the data of the sm...
We present results of an improved analysis of the experimental data of the EAS Cherenkov array Tunka...
Arrival directions of ultra-high energy cosmic rays (UHECRs) in the equatorial system, detected with...
We present results of an improved analysis of the experimental data of the EAS Cherenkov array Tunka...
Abstract: The two-point autocorrelation function of ultrahigh energy cosmic ray (UHECR) arrival dire...
We report a first result on the cosmic ray energy spectrum above 3 \Theta 10 18 eV measured by the...
We measure the spectrum of cosmic rays with energies greater than 10 18.2 eV with the fluorescence d...
The cosmic ray energy spectrum in the range E-o = 10(15)-10(16) eV (including the region of the stee...
The break observed in the electron shower size power law spectrum of Extensive Air Showers (EAS) at ...
[著者版]We present an updated all-particle energy spectrum of primary cosmic rays in a wide range from ...
International audienceThe two-point autocorrelation function of ultra-high energy cosmic ray (UHECR)...
In this work the energy spectrum of cosmic rays based on Yakutsk EAS array data is presented. After ...
The experimental data on the cosmic ray energy spectrum obtained from the Small Cherenkov Array in Y...
The Yakutsk array observes the Cherenkov light emitted by UHECR in atmosphere. Recently, an autonomo...
The experimental data on the cosmic ray energy spectrum obtained from the Small Cherenkov Array in Y...
A spectrum of cosmic rays within energy range 1015 − 3 × 1017 eV was derived from the data of the sm...
We present results of an improved analysis of the experimental data of the EAS Cherenkov array Tunka...
Arrival directions of ultra-high energy cosmic rays (UHECRs) in the equatorial system, detected with...
We present results of an improved analysis of the experimental data of the EAS Cherenkov array Tunka...
Abstract: The two-point autocorrelation function of ultrahigh energy cosmic ray (UHECR) arrival dire...
We report a first result on the cosmic ray energy spectrum above 3 \Theta 10 18 eV measured by the...
We measure the spectrum of cosmic rays with energies greater than 10 18.2 eV with the fluorescence d...
The cosmic ray energy spectrum in the range E-o = 10(15)-10(16) eV (including the region of the stee...
The break observed in the electron shower size power law spectrum of Extensive Air Showers (EAS) at ...
[著者版]We present an updated all-particle energy spectrum of primary cosmic rays in a wide range from ...
International audienceThe two-point autocorrelation function of ultra-high energy cosmic ray (UHECR)...