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Dive into the research topics where A. N. Kurenya is active.

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Featured researches published by A. N. Kurenya.


arXiv: Astrophysics | 2006

EMMA: A new underground cosmic-ray experiment

T. Enqvist; V Föhr; J. Joutsenvaara; T Jämsén; P. Keränen; P. Kuusiniemi; H. Laitala; M Lehtola; A. Mattila; J Narkilahti; J Peltoniemi; H. Remes; M Reponen; T. Räihä; J. Sarkamo; C Shen; M. Vaittinen; Z Zhang; L. Ding; Q Zhu; Matts Roos; I. M. Dzaparova; S. N. Karpov; A. N. Kurenya; V. B. Petkov; A. F. Yanin; H. O. U. Fynbo

A cosmic-ray experiment of new type is under construction in the Pyhasalmi mine in the underground laboratory of the University of Oulu, Finland. It aims to study the composition of cosmic rays at and above the knee region (energy above 1 PeV). The experiment, called EMMA, covers about 150 m2 of detector area, and the setup is capable of measuring the multiplicity and the lateral distribution of underground muons, and the arrival direction of the air shower. The detector is placed at the depth of about 85 metres (corresponding about 240 mwe) which gives a threshold energy of muons of about 45 GeV. The rock overburden filters out all other particles of the air shower except the high-energy muons. These high-energy muons originate at high altitudes close to the first interaction of the primary cosmic ray and they carry more information about the primary than low-energy muons. The full-size detector is supposed to run by the end of 2007.


Physics of Particles and Nuclei | 2018

Scintillation detector with SiPM matrix as a photosensor

I. M. Dzaparova; V. I. Volchenko; A. M. Gangapshev; E. A. Gorbacheva; A. N. Kurenya; V. B. Petkov; A. V. Sergeev; A. F. Yanin

The results of a characterization study of the scintillation detector with SiPM matrices as multichannel photosensors are presented. The SiPM matrix attached to a plastic scintillator gives a snapshot of the glowing track of a charged particle traversing the scintillator.


Physics of Particles and Nuclei | 2018

Search for Neutrino Bursts at the Baksan Underground Scintillation Telescope

R. V. Novoseltseva; M. M. Boliev; I. M. Dzaparova; M. M. Kochkarov; A. N. Kurenya; Yu. F. Novoseltsev; V. B. Petkov; V. I. Volchenko; G. V. Volchenko; A. F. Yanin

The Baksan Underground Scintillation Telescope has been operating under the program of searching for neutrino bursts since the middle of 1980. The target is two parts of the facility with the total mass of 240 t. The actual observation time over the period from June 30, 1980, to December 31, 2016, is 31.27 years. No candidate for the stellar core collapse has been detected during the observation period. The upper bound for the mean rate of the supernova core collapse in our Galaxy is 0.074 y


Physics of Particles and Nuclei | 2018

Development of the Scintillation Track Detector Based on Multichannel Photodetectors

A. F. Yanin; I. M. Dzaparova; E. A. Gorbacheva; A. N. Kurenya; V. B. Petkov; A. V. Sergeev


Physics of Particles and Nuclei | 2018

The Carpet-3 Multipurpose Air Shower Array of the Baksan Neutrino Observatory of the Institute for Nuclear Research, Russian Academy of Sciences

D. D. Dzhappuev; V. I. Volchenko; G. V. Volchenko; E. A. Gorbacheva; I. M. Dzaparova; A. U. Kudzhaev; A. N. Kurenya; N. F. Klimenko; A. S. Lidvansky; O. I. Mikhailova; V. B. Petkov; M. M. Khadzhiev; A. F. Yanin

^{{ - 1}}


Physics of Particles and Nuclei | 2018

Prototype Scintillation Detector with Photosensors Based on Silicon Photomultiplier Arrays

I. M. Dzaparova; A. F. Yanin; E. A. Gorbacheva; A. N. Kurenya; V. B. Petkov; A. V. Sergeev


Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017) | 2017

The search for neutrino bursts from supernovae at the Baksan Underground Scintillation Telescope; 36 years of exposure

Valeriy Petkov; M. M. Kochkarov; Musa M. Boliev; I. M. Dzaparova; A. N. Kurenya; Yu.F. Novoseltsev; R. V. Novoseltseva; P. S. Striganov; Vladimir I. Volchenko; G. V. Volchenko; A. F. Yanin

(90% CL).


Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017) | 2017

Search for diffuse gamma radiation with energy > 100 TeV at the Carpet-3 experiment

Valeriy Petkov; A. S. Lidvansky; D.D. Dzhappuev; Vladimir I. Volchenko; G. V. Volchenko; E.A. Gorbacheva; I. M. Dzaparova; N.F. Klimenko; A.U. Kudzhaev; A. N. Kurenya; O.I. Mikhailova; M.M. Khadzhiev; A. F. Yanin

Matrices of silicon photomultipliers (SiPM) are promising multichannel photosensors for scintillation detectors. They can be used to construct tracks of relativistic particles inside detectors. The first detectors based on the direct contact of the SiPM matrices with the surface of the scintillation detector and with the application of Fresnel lenses are developed; promising variants of large detectors for neutrino astrophysics and geophysics are proposed.


Measurement Techniques | 2017

Multichannel Measurement System for Data Acquisition From Silicon Photomultiplier Arrays

A. F. Yanin; I. M. Dzaparova; V. I. Volchenko; E. A. Gorbacheva; A. N. Kurenya; V. B. Petkov

An experiment for measuring the flux of cosmic gamma rays with energy above 100 TeV is currently being prepared at the Baksan Neutrino Observatory of the Institute for Nuclear Research, Russian Academy of Sciences. For this purpose, based on the Carpet-2 shower array which has been operating for many years, the Carpet-3 multipurpose shower array is being constructed. In particular, the preparation of the experiment supposes an increase in the area of the muon detector (MD) and ground part of the array. For ground modules of the Carpet-3 array, a scintillation detector with a liquid scintillator in a plastic package has been elaborated. In this work, descriptions of the Carpet-3 array and working characteristics of the new scintillation detector are presented.


Physics of Particles and Nuclei | 2018

Hardware and Software for the Data Aсquisition Systems of the Andyrchi and Carpet-3 Air Shower Facilities

A. N. Kurenya; I. S. Savanov; V. B. Petkov; A. V. Sergeev; D. D. Dzhappuev; V. B. Puzin; S. A. Naroenkov; I. M. Dzaparova; A. F. Yanin; M. A. Nalivkin

A prototype scintillation detector with photosensors based on silicon photomultiplier (SiPM) arrays is described. Such a method of data-taking will make it possible to obtain an image (snapshot) of the event and, thereby, to separate different types of events (particle interactions) in the detector. For this purpose, the characteristics of SiPMs have been studied and a calibration measurement technique developed.

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A. F. Yanin

Russian Academy of Sciences

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I. M. Dzaparova

Russian Academy of Sciences

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V. B. Petkov

Russian Academy of Sciences

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E. A. Gorbacheva

Russian Academy of Sciences

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G. V. Volchenko

Russian Academy of Sciences

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A. V. Sergeev

Russian Academy of Sciences

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V. I. Volchenko

Russian Academy of Sciences

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M. M. Kochkarov

Russian Academy of Sciences

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R. V. Novoseltseva

Russian Academy of Sciences

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A. S. Lidvansky

Russian Academy of Sciences

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