11 citations · 58 across the 24 of their papers we have counts for
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Parallel Version of CORSIKA Code with Cherenkov Option for SPHERE-3 Project
M. D. Ziva, V. I. Galkin, E. A. Bonvech +7
We use Lomonosov-2 supercomputing facility for the generation of extensive air shower events with Cherenkov light which is a rather time consuming procedure. At primary energies sl…
A Multi-Level Parallel Pipeline for SPHERE-3 Detector Simulation: From EAS Generation to Image Approximation
V. A. Ivanov, V. I. Galkin, E. A. Bonvech +7
Optimization of the SPHERE-3 detector configuration, designed to study the mass composition of primary cosmic rays in the energy range 1--1000 PeV by registering Cherenkov light re…
The project of a ground-based wide-angle EAS Cherenkov light imaging detector for PCR mass composition study in the 1-1000 PeV energy range
D. V. Chernov, E. A. Bonvech, O. V. Cherkesova +9
This report presents a draft of a new detector designed to determine the chemical composition of primary cosmic rays based on the characteristics of the angular distribution of Che…
Four years of wide-field search for nanosecond optical transients with the TAIGA-HiSCORE Cherenkov array
A. D. Panov, I. I. Astapov, G. M. Beskin +75
It has been previously demonstrated [Panov et al. Physics of Atomic Nuclei 84(2021)1037] that the TAIGA-HiSCORE Cherenkov array, originally built for cosmic ray physics and ultrahi…
Software Suite for Modeling Cherenkov Images of Extensive Air Showers in the SPHERE-3 Detector
V. A. Ivanov, V. I. Galkin, E. A. Bonvech +7
The study of cosmic rays in the energy range from 1 to 1000 PeV is crucial for understanding their origins and propagation paths. As part of this research, a new SPHERE-3 installat…
Application of convolutional neural networks for extensive air shower separation in the SPHERE-3 experiment
E. L. Entina, D. A. Podgrudkov, C. G. Azra +9
A new SPHERE-3 telescope is being developed for cosmic rays spectrum and mass composition studies in the 5--1000 PeV energy range. Registration of extensive air showers using refle…
TAIGA -- an advanced hybrid detector complex for astroparticle physics and high energy gamma-ray astronomy
N. M. Budnev, I. Astapov, P. Bezyazeekov +74
The physical motivations, present status, main results in study of cosmic rays and in the field of gamma-ray astronomy as well future plans of the TAIGA-1 (Tunka Advanced Instrumen…
The Tunka-Grande scintillation array: current results
A. L. Ivanova, I. Astapov, P. Bezyazeekov +76
The Tunka-Grande experiment is a scintillation array with about 0.5 sq.km sensitive area at Tunka Valley, Siberia, for measuring charged particles and muons in extensive air shower…
Search for Astrophysical Nanosecond Optical Transients with TAIGA-HiSCORE Array
A. D. Panov, I. I. Astapov, A. K. Awad +81
A wide-angle Cerenkov array TAIGA-HiSCORE (FOV 0.6 sr), was originally created as a part of TAIGA installation for high-energy gamma-ray astronomy and cosmic ray physics. Arr…
Investigation of energy spectrum and chemical composition of primary cosmic rays in 1-100 PeV energy range with a UAV-borne installation
D. Chernov, E. Bonvech, M. Finger +5
A new project is developed with the implementation of a relatively new method of studying the primary cosmic ray -- the registration of extensive air showers' optical Vavilov-Chere…
The SPHERE-2 detector for observation of extensive air showers in 1 PeV -- 1 EeV energy range
R. A. Antonov, E. A. Bonvech, D. V. Chernov +6
The SPHERE-2 balloon-borne detector designed for extensive air shower (EAS) observations using EAS optical Vavilov-Cherenkov radiation (``Cherenkov light''), reflected from the sno…
Spatial and temporal structure of EAS reflected Cherenkov light signal
R. A. Antonov, E. A. Bonvech, D. V. Chernov +4
A compact device lifted over the ground surface might be used to observe optical radiation of extensive air showers (EAS). Here we consider spatial and temporal characteristics of…
Status of the SPHERE experiment
R. A. Antonov, S. P. Beschapov, E. A. Bonvech +11
Here is presented the current state of the SPHERE-2 balloon-borne experiment. The detector is elevated up to 1 km above the snow surface and registers the reflected Vavilov-Cherenk…