We present the main results of the Extensive Air Shower Cherenkov array Tunka-25. They cover the energy spectrum from 8 · 1014 to 1017 eV and mass composition of primary cosmic rays in the energy range of 3·1015 − 3 · 1016 eV. A new lateral distribution function (LDF) of Air Shower Cherenkov light and a new method to analyze the maximum depth distribution of the shower have been developed. Both have been successfully applied in the data analysis of Tunka-25. We also discuss methods of time and amplitude calibration of the array, providing an accurate determination of the primary energy and the steepness of the LDF
The Yakutsk array observes the Cherenkov light emitted by UHECR in atmosphere. Recently, an autonomo...
Tunka-Rex is a radio detector for cosmic-ray air showers in Siberia, triggered by Tunka-133, a co-lo...
The Cherenkov light array for the registration of extensive air showers (EAS) Tunka-133 collected da...
We present results of an improved analysis of the experimental data of the EAS Cherenkov array Tunka...
We present results of an improved analysis of the experimental data of the EAS Cherenkov array Tunka...
The Tunka-133 Cherenkov complex for recording extensive air showers (EAS) collected data over seven ...
The Cherenkov light lateral distribution function (LDF) was simulated with the CORSIKAcode in the...
Abstract. The Lateral distribution function of Cherenkov radiation from particles of Extensive Air S...
The EAS Cherenkov light array Tunka-133, with ~ 3 km 2 geometric area, is taking data since 2009.T...
The extensive air shower Cherenkov light array Tunka-133 collected data during 7 winter seasons from...
Data obtained with two detectors located at the Tunka Cosmic Ray facility are presented. The Cherenk...
New results of 300 hours of operation of the Tunka array are presented. An improved parametrization ...
The project of an EAS Cherenkov array in the Tunka valley/Siberia with an area of about 1 km^2 is pr...
A corrected energy dependence of the depth of the maximum in the wide range of energies 10$^{15}$ to...
The Tunka Radio Extension (Tunka-Rex) is a radio detector at the TAIGA facility located in Siberia n...
The Yakutsk array observes the Cherenkov light emitted by UHECR in atmosphere. Recently, an autonomo...
Tunka-Rex is a radio detector for cosmic-ray air showers in Siberia, triggered by Tunka-133, a co-lo...
The Cherenkov light array for the registration of extensive air showers (EAS) Tunka-133 collected da...
We present results of an improved analysis of the experimental data of the EAS Cherenkov array Tunka...
We present results of an improved analysis of the experimental data of the EAS Cherenkov array Tunka...
The Tunka-133 Cherenkov complex for recording extensive air showers (EAS) collected data over seven ...
The Cherenkov light lateral distribution function (LDF) was simulated with the CORSIKAcode in the...
Abstract. The Lateral distribution function of Cherenkov radiation from particles of Extensive Air S...
The EAS Cherenkov light array Tunka-133, with ~ 3 km 2 geometric area, is taking data since 2009.T...
The extensive air shower Cherenkov light array Tunka-133 collected data during 7 winter seasons from...
Data obtained with two detectors located at the Tunka Cosmic Ray facility are presented. The Cherenk...
New results of 300 hours of operation of the Tunka array are presented. An improved parametrization ...
The project of an EAS Cherenkov array in the Tunka valley/Siberia with an area of about 1 km^2 is pr...
A corrected energy dependence of the depth of the maximum in the wide range of energies 10$^{15}$ to...
The Tunka Radio Extension (Tunka-Rex) is a radio detector at the TAIGA facility located in Siberia n...
The Yakutsk array observes the Cherenkov light emitted by UHECR in atmosphere. Recently, an autonomo...
Tunka-Rex is a radio detector for cosmic-ray air showers in Siberia, triggered by Tunka-133, a co-lo...
The Cherenkov light array for the registration of extensive air showers (EAS) Tunka-133 collected da...