15 citations · 21 across the 15 of their papers we have counts for
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The PRISMA-36 array for studying variations of the thermal neutron flux
M. B. Amelchakov, A. Chiavassa, D. M. Gromushkin +11
From 2012 to 2023, the PRISMA-32 array was in operation at the Experimental Complex NEVOD (MEPhI, Moscow). The purpose of the array was to study extensive air showers by detecting…
Calibration of the NEVOD-EAS array for detection of extensive air showers
M. B. Amelchakov, A. G. Bogdanov, A. Chiavassa +14
In this paper we discuss the calibration of the NEVOD-EAS array which is a part of the Experimental Complex NEVOD, as well as the results of studying the response features of its s…
Testing the new QSM-6M optical module with the NEVOD Cherenkov water detector
S. S. Khokhlov, T. A. Karetnikova, V. V. Kindin +3
The method for studying characteristics of the response of optical modules of neutrino telescopes to various classes of events registered in the volume of the Cherenkov water detec…
The NEVOD-EAS air-shower array
M. B. Amelchakov, N. S. Barbashina, A. G. Bogdanov +14
The Experimental complex NEVOD includes several different setups for studying various components of extensive air showers (EAS) in the energy range from 10^10 to 10^18 eV. The NEVO…
New detectors of the Experimental complex NEVOD for multicomponent EAS detection
I. I. Yashin, N. S. Barbashina, A. A. Borisov +10
Experimental complex (EC) NEVOD includes a number of unique experimental facilities for studies of main components of cosmic rays on the Earth's surface. The complex is used for th…
Detection of extensive air showers with the NEVOD-EAS cluster type detector
I. A. Shulzhenko, M. B. Amelchakov, N. S. Barbashina +13
A new cluster type shower array NEVOD-EAS is designed for estimating the size, axis position and arrival direction of extensive air showers registered by the Cherenkov water detect…
Energy characteristics of multi-muon events in a wide range of zenith angles
A. G. Bogdanov, N. S. Barbashina, D. V. Chernov +13
Change of the energy characteristics of muon bundles with an increase of the primary cosmic ray particles energy can be a key to solving the problem of muon excess in the extensive…