Search

Your search keyword '"S. F. Berezhnev"' showing total 12 results
Start Over Author "S. F. Berezhnev"
12 results on '"S. F. Berezhnev"'

1. First results from the operation of the prototype Tunka-HiSCORE array

Author

S. F. Berezhnev, N. M. Budnev, M. Büker, M. Brückner, R. Wischnewski, A. V. Gafarov, O. A. Gress, T. Gress, A. N. Dyachok, S. N. Epimakhov, A. V. Zagorodnikov, V. L. Zurbanov, N. N. Kalmykov, N. I. Karpov, E. N. Konstantinov, E. E. Korosteleva, V. A. Kozhin, M. Kunnas, L. A. Kuzmichev, A. Chiavassa, B. K. Lubsandorzhiev, N. B. Lubsandorzhiev, R. R. Mirgazov, R. D. Monkhoev, R. Nachtigall, A. L. Pakhorukov, M. I. Panasyuk, L. V. Pankov, A. Porelli, V. A. Poleshchuk, E. G. Popova, V. V. Prosin, V. S. Ptuskin, M. Rueger, G. I. Rubtsov, Yu. A. Semeney, A. A. Silaev, A. V. Skurikhin, L. G. Sveshnikova, M. Tluczykont, D. Hampf, D. Horns, and O. A. Chvalaev

Subjects
Physics, Data processing, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Gamma ray, General Physics and Astronomy, Astronomy, Cosmic ray, Differential spectrum, Observatory, Angle of arrival, Cherenkov radiation, Energy (signal processing), Remote sensing
Abstract

The Tunka-HISCORE wide-angle Cherenkov array, one part of the planned TAIGA integrated gamma observatory intended for investigations in the field of high-energy (>30 TeV) gamma-ray astronomy and cosmic-ray physics, is deployed in the Tunka Valley (Buryat Republic). The first results from operating a prototype array composed of nine stations spread over an area of ∼0.1 square kilometers during the winter of 2013–2014 are presented. Data processing techniques are described, along with data on the accuracy of reconstructing the position of a shower’s axis, energy, and angle of arrival. The differential spectrum of all cosmic-ray particles in a shower in the energy range of 2 × 1014 to 2 × 1016 eV is presented and compared to the available data.

Published
2015
Full Text
View/download PDF

2. Energy spectrum and mass composition of cosmic rays, by the data of the Tunka-133 array

Author

S. F. Berezhnev, N. M. Budnev, O. A. Gress, A. N. Dyachok, S. N. Epimakhov, A. V. Zagorodnikov, N. N. Kalmykov, N. I. Karpov, V. A. Kozhin, E. N. Konstantinov, A. V. Korobchenko, E. E. Korosteleva, L. A. Kuzmichev, A. Chiavassa, B. K. Lubsandorzhiev, N. B. Lubsandorzhiev, R. R. Mirgazov, R. D. Monkhoev, E. A. Osipova, M. I. Panasyuk, L. V. Pankov, A. L. Pakhorukov, E. G. Popova, V. V. Prosin, V. S. Ptuskin, L. G. Sveshnikova, Yu. A. Semeney, A. A. Silaev, A. V. Skurikhin, O. A. Chvalaev, C. Spiering, and I. V. Yashin

Subjects
Core (optical fiber), Physics, Range (particle radiation), Air shower, Primary energy, General Physics and Astronomy, Direction of arrival, Cosmic ray, Astrophysics, Energy (signal processing), Cherenkov radiation, Computational physics
Abstract

The Tunka-133 Cherenkov light array for the detection of extensive air showers (EAS) acquires data over the five winters from 2009 to 2014. The direction of arrival, the shower core coordinates on the plane of observation, the primary energy, and the depth of the shower maximum are reconstructed for each EAS. A differential all-particle energy spectrum is obtained in the energy range of 6 × 1015–3 × 1018 eV over 1540 h, along with the energy dependence of the average depth of the shower maximum in the range of 6 × 1016–3 × 1018 eV. Based on this dependence, the variation in the average composition of the primary cosmic rays is estimated as a function of energy.

Published
2015
Full Text
View/download PDF

3. The Primary CR Spectrum by the Data of the Tunka-133 Array

Author

S. F. Berezhnev, N. M. Budnev, A. Chiavassa, O. A. Chvalaev, O. A. Gress, T. I. Gress, A. N. Dyachok, S. N. Epimakhov, N. I. Karpov, N. N. Kalmykov, E. N. Konstantinov, A. V. Korobchenko, E. E. Korosteleva, V. A. Kozhin, L. A. Kuzmichev, B. K. Lubsandorzhiev, N. B. Lubsandorzhiev, R. R. Mirgazov, R. D. Monkhoev, E. A. Osipova, A. L. Pakhorukov, M. I. Panasyuk, L. V. Pankov, E. G. Popova, V. V. Prosin, V. S. Ptuskin, Yu. A. Semeney, A. A. Silaev, A. V. Skurikhin, C. Spiering, L. G. Sveshnikova, and A. V. Zagorodnikov

Subjects
Physics, Data acquisition, Calibration (statistics), Primary (astronomy), Energy spectrum, Astronomy, Astrophysics, Spectrum (topology)
Published
2016
Full Text
View/download PDF

4. The hardware of the HiSCORE γ-ray and cosmic ray Cherenkov detector

Author

M. Kunnas, R. Nachtigall, S. N. Epimakhov, M. Tluczykont, L. A. Kuzmichev, S. F. Berezhnev, N. M. Budnev, M. Büker, A. Chiavassa, O. B. Chvalaev, O. A. Gress, A. N. Dyachok, U. Einhaus, D. Hampf, D. Horns, A. Ivanova, N. I. Karpov, N. N. Kalmykov, E. N. Konstantinov, A. V. Korobchenko, E. E. Korosteleva, V. A. Kozhin, B. K. Lubsandorzhiev, N. B. Lubsandorzhiev, R. R. Mirgazov, A. Pakhorukov, M. I. Panasyuk, L. V. Pankov, V. Poleschuk, E. G. Popova, V. V. Prosin, V. S. Ptuskin, G. P. Rowell, Yu. A. Semeney, B. A. Shaibonov (junior), A. A. Silaev, A. A. Silaev (junior), A. V. Skurikhin, C. Spiering, L. G. Sveshnikova, R. Wischnewski, I. V. Yashin, and A. V. Zagorodnikov

Subjects
Physics, Photomultiplier, COSMIC cancer database, business.industry, Cherenkov detector, Gamma ray, Astronomy, Single station, Cosmic ray, First light, law.invention, Air shower, law, business, Computer hardware
Abstract

The HiSCORE (Hundred Square km Cosmic ORigin Explorer) project is a ground-based large-area wideangle air shower detector array that will measure gamma rays and cosmic rays in the energy range of 10 TeV up to 1EeV. Each detector array station consists of four separate light collectors with an 8-inch photomultiplier (PMT) at each end. The first station prototype has already been deployed to Tunka valley. On-site station integration and first measurements have been made. This poster will focus on the hardware aspects and the first light results of the single station.

Published
2012
Full Text
View/download PDF

5. Tunka-133: the New EAS Cherenkov Light Array for Cosmic Ray Study

Author

Yu. A. Semeney, B. A. M. Shaibonov, L. G. Sveshnikova, B. V. Antokhonov, V. S. Ptuskin, E. N. Konstantinov, C. Spiering, A. Chiavassa, S. F. Berezhnev, O. A. Gress, I. V. Yashin, L. V. Pankov, J. Snyder, V. A. Kozhin, M. Stockham, B. K. Lubsandorzhiev, N. N. Kalmykov, V. V. Prosin, A. V. Skurikhin, N. M. Budnev, M. I. Panasyuk, R. R. Mirgazov, A. V. Zablotsky, A.V. Korobchenko, A. N. Dyachok, E.G. Popova, A. A. Silaev, A. V. Zagorodnikov, N. I. Karpov, O. A. Chvalaiev, E. E. Korosteleva, D. Z. Besson, L. A. Kuzmichev, and R. Wischnewski

Subjects
Physics, Astronomy, Cosmic ray, Cherenkov radiation
Published
2011
Full Text
View/download PDF

6. TUNKA-133: A new array for the study of ultra-high energy cosmic rays

Author

B. V. Antokhonov, S. F. Berezhnev, D. Besson, N. M. Budnev, R. Wischnevski, O. A. Gress, A. N. Diachok, A. V. Zablotsky, A. V. Zagorodnikov, N. N. Kalmykov, N. I. Karpov, V. A. Kozhin, E. E. Korosteleva, A. V. Korobchenko, L. A. Kuzmichev, A. Chiavassa, B. K. Lubsandorzhiev, R. R. Mirgazov, M. I. Panasyuk, L. V. Pankov, V. V. Prosin, V. S. Ptuskin, Yu. A. Semeney, A. A. Silaev, A. V. Skurikhin, M. Stokham, O. A. Chvalaiev, B. A. Shaibonov, J. Snyder, Ch. Spiering, and I. V. Yashin

Subjects
Physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, General Physics and Astronomy, Cosmic ray, Ultra-high-energy cosmic ray, Astrophysics, Cherenkov radiation
Abstract

A new array for studying ultra-high energy cosmic rays was inaugurated in 2009 in the Tunka Valley, about 50 km from Lake Baikal. Having an area of 1 km2, the new facility allows us to study cosmic rays with energies of 1015–1018 eV via the a unified method for registering Cherenkov radiation from extensive air showers (EASes) and is making a substantial contribution to understanding the origin of ultra-high energy cosmic rays. We describe the current state of the experiment, the new methodological approach, our initial results, and the plans for further development of the array.

Published
2011
Full Text
View/download PDF

7. The Gigaton Volume Detector in Lake Baikal

Author

I. A. Belolaptikov, M.B. Milenin, B. Shoibonov, I. A. Danilchenko, K.V. Golubkov, V. A. Poleschuk, A. I. Panfilov, A. Pan'kov, A. A. Perevalov, M.I. Rozanov, A. N. Dyachok, V. I. Lyashuk, E. A. Osipova, Ch. Spiering, N. M. Budnev, T.I. Gres, D. P. Petukhov, V. M. Aynutdinov, O. G. Grishin, S.V. Fialkovsky, O. N. Gaponenko, V. A. Zhukov, V.F. Kulepov, A.D. Avrorin, E.G. Popova, Olga Suvorova, A. A. Sheifler, A. I. Klimov, G.V. Domogatsky, E.N. Pliskovsky, L. V. Pankov, O. Gres, A. M. Klabukov, A. Kochanov, R. R. Mirgazov, E. Middell, E. V. Ryabov, A. V. Shirokov, B.A. Tarashansky, S. F. Berezhnev, R. Wischnewski, A.P. Koshechkin, Aleksey Zagorodnikov, D. Bogorodsky, K.V. Konischev, A. A. Doroshenko, Zh.-A.M. Dzhilkibaev, V. V. Prosin, N. Grishin, G. Ermakov, A.V. Korobchenko, V. Rubtzov, D.A. Kuleshov, A. S. Yagunov, L. A. Kuzmichev, and S. Mikheyev

Subjects
Physics, Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Volume (computing), Astronomy, law.invention, Telescope, Observatory, law, ddc:530, Sensitivity (control systems), Neutrino, Nonlinear Sciences::Pattern Formation and Solitons, Instrumentation, Underwater acoustic communication
Abstract

The objective of the Baikal Project is the creation of a kilometer-scale high-energy neutrino observatory: the Gigaton Volume Detector (GVD) in Lake Baikal. Basic elements of the GVD – new optical modules, FADC readout units, and underwater communication systems – were investigated and tested in Lake Baikal with prototype strings in 2008–2010. We describe the results of prototype strings operation and review the preliminary design and expected sensitivity of the GVD telescope.

Published
2011
Full Text
View/download PDF

8. The Baikal neutrino experiment

Author

A. Pan'kov, Olga Suvorova, A. I. Panfilov, L. V. Pankov, M.I. Rozanov, V. M. Aynutdinov, O. N. Gaponenko, A.D. Avrorin, G.V. Domogatsky, S. F. Berezhnev, E.N. Pliskovsky, A. M. Klabukov, S.V. Fialkovsky, K.V. Konischev, N. M. Budnev, A. I. Klimov, A. V. Zagorodnikov, V. A. Zhukov, O. G. Grishin, D. P. Petukhov, V. A. Poleschuk, Ralf Wischnewski, L. A. Kuzmichev, I. A. Danilchenko, O. Gres, A. N. Dyachok, S. Mikheyev, N. Grishin, T.I. Gres, V.A. Balkanov, B. Shoibonov, G. Ermakov, B.A. Tarashansky, E. Middell, Ch. Spiering, A.P. Koshechkin, A. Kochanov, R. R. Mirgazov, A. V. Shirokov, E. A. Osipova, D.A. Kuleshov, E.G. Popova, A. A. Doroshenko, Zh.-A.M. Dzhilkibaev, V.F. Kulepov, V. V. Prosin, A.V. Korobchenko, P. G. Pokhil, V. Rubtzov, A.A. Sheifler, M.B. Milenin, D. Bogorodsky, I. A. Belolaptikov, K.V. Golubkov, and A. S. Yagunov

Subjects
Physics, Nuclear physics, Nuclear and High Energy Physics, Astronomy, Flux, ddc:530, Neutrino astronomy, Neutrino, Instrumentation
Abstract

We review the status of the Lake Baikal Neutrino Experiment. Preparation towards a km3-scale Gigaton Volume Detector (GVD) in Lake Baikal is currently a central activity. As an important milestone, a km3-prototype string comprising of 12 optical modules and based on a completely new technology, has been installed and was put in operation together with NT200+ in April, 2009. We also present recent results from the long-term operation of NT200, including an improved limit on the diffuse astrophysical neutrino flux.

Published
2011
Full Text
View/download PDF

9. Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype

Author

Yu. A. Semeney, A. Pakhorukov, A. V. Skurikhin, V. A. Poleschuk, R. Nachtigall, O. A. Gress, A. V. Gafarov, M. Kunnas, A.V. Zurbanov, A. Porelli, S. Kiryuhin, Dieter Horns, V. A. Kozhin, C. Spiering, Bayarto Lubsandorzhiev, M. Tluczykont, M. I. Panasyuk, M. Rüger, A.V. Dyachok, L. G. Sveshnikova, A. Chiavassa, V. Prosin, S. F. Berezhnev, A.V. Korobchenko, S. Epimakhov, V. S. Ptuskin, E. E. Korosteleva, L. V. Pankov, R. D. Monkhoev, T. I. Gress, Aleksey Zagorodnikov, N. B. Lubsandorzhiev, N. I. Karpov, Grigory Rubtsov, N. N. Kalmykov, N. M. Budnev, L. A. Kuzmichev, A. A. Silaev, R. Wischnewski, E. N. Konstantinov, E.G. Popova, R. R. Mirgazov, V. Samoliga, O.A. Chvalaev, M. Brückner, and E. A. Osipova

Subjects
Physics, 010308 nuclear & particles physics, Maximum depth, QC1-999, 0103 physical sciences, Energy spectrum, Cosmic ray, Astrophysics, 010306 general physics, 01 natural sciences, Cherenkov radiation, Remote sensing
Abstract

Data obtained with two detectors located at the Tunka Cosmic Ray facility are presented. The Cherenkov light array for registration of extensive air showers (EAS) Tunka-133 collected data during 5 winter seasons since 2009 to 2014. The differential energy spectrum of all particles and the dependence of the average maximum depth on the energy in the range of 6 · 10 15 −10 18 eV measured for 1540 hours of observation are presented.The preliminary all particle energy spectrum by the data of Tunka-HiSCORE prototype array, installed in 2013, is presented. Some additional experiments in the Tunka Valley are briefly described.

Published
2016
Full Text
View/download PDF

10. Primary CR energy spectrum and mass composition by the data of Tunka-133 array

Author

A. Chiavassa, V. Prosin, A. A. Silaev, A. Pakhorukov, R. D. Monkhoev, T. I. Gress, Bayarto Lubsandorzhiev, L. A. Kuzmichev, N. N. Kalmykov, A. V. Skurikhin, E. N. Konstantinov, V. S. Ptuskin, A.V. Dyachok, E. E. Korosteleva, S. Epimakhov, S. F. Berezhnev, O. A. Gress, A.V. Korobchenko, L. G. Sveshnikova, V. A. Kozhin, O.A. Chvalaev, E. A. Osipova, Mikhail Panasyuk, N. I. Karpov, E.G. Popova, N. M. Budnev, N. B. Lubsandorzhiev, R. R. Mirgazov, L. V. Pankov, C. Spiering, Aleksey Zagorodnikov, Yu. A. Semeney, and Silaev, A. A.

Subjects
Physics, Nuclear physics, Range (particle radiation), Maximum depth, Primary (astronomy), QC1-999, Energy spectrum, ddc:530, Mass composition, Energy (signal processing), Cherenkov radiation
Abstract

The Cherenkov light array for the registration of extensive air showers (EAS) Tunka-133 collected data during 5 winter seasons from 2009 to 2014. The differential energy spectrum of all particles and the dependence of the average maximum depth on the energy in the range of 6 · 10 15 -10 18 eV measured for 1540 hours of observation are presented.

Published
2015
Full Text
View/download PDF

11. Status of the BAIKAL neutrino experiment

Author

V.F. Kulepov, A. A. Perevalov, R. Wischnewski, O. G. Grishin, A. S. Yagunov, D. A. Petukhov, O. N. Gaponenko, R. R. Mirgazov, D.Yu. Bogorodsky, A. I. Klimov, E. Middell, O. A. Gress, B. Shoibonov, Evgenii V Rjabov, B. A. Tarashchansky, A. V. Zagorodnikov, A. A. Doroshenko, E. A. Osipova, Zh.-A.M. Dzhilkibaev, V. V. Prosin, I. A. Danilchenko, V. A. Balkanov, M.B. Milenin, E.N. Pliskovsky, A. M. Klabukov, A.V. Avrorin, K.V. Golubkov, Ch. Spering, I. A. Belolaptikov, G. Ermakov, A. N. Dyachok, S.V. Fialkovsky, V. Rubzov, A. I. Panfilov, V. A. Zhukov, M.I. Rozanov, A.P. Koshechkin, V.I. Ljashuk, A.V. Korobchenko, A. Pan'kov, T. I. Gress, A. A. Sheifler, V. Poleshchuk, E.G. Popova, G.V. Domogatsky, V. M. Aynutdinov, N. Grishin, A. V. Shirokov, Olga Suvorova, S. F. Berezhnev, L. V. Pankov, N. M. Budnev, L. A. Kuzmichev, K. V. Konishchev, D.A. Kuleshov, and S. P. Mikheev

Subjects
Physics, Neutrino telescope, General Physics and Astronomy, Astronomy, Astrophysics, Neutrino
Abstract

The development of the NT1000 km3 neutrino telescope at Lake Baikal has been the main goal of the BAIKAL collaboration since 2006. This work presents selected results obtained in the course of developing and testing key elements and systems of the future detector.

Published
2011
Full Text
View/download PDF

12. First deployment and prototype data of HiSCORE

Author

R Nachtigall, M Kunnas, S N Epimakhov, M Tluczykont, L A Kuzmichev, S F Berezhnev, N M Budnev, M Büker, A Chiavassa, O B Chvalaev, O A Gress, A N Dyachok, U Einhaus, D Hampf, D Horns, A Ivanova, N I Karpov, N N Kalmykov, E N Konstantinov, A V Korobchenko, E E Korosteleva, V A Kozhin, B K Lubsandorzhiev, N B Lubsandorzhiev, R R Mirgazov, A Pakharukov, M I Panasyuk, L V Pankov, V Poleschuk, E G Popova, V V Prosin, V S Ptuskin, G P Rowell, Yu A Semeney, B A Shaibonov, A A Silaev, A A Silaev (junior), A V Skurikhin, C Spiering, L G Sveshnikova, R Wischnewski, I V Yashin, and A V Zagorodnikov

Subjects
Physics, History, Photomultiplier, COSMIC cancer database, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Gamma ray, Astronomy, Cosmic ray, Computer Science Applications, Education, Data acquisition, Air shower, Sky, media_common
Abstract

With the HiSCORE (Hundred*i Square kilometer Cosmic ORigin Explorer) experiment we aim at the exploration of the accelerator sky using indirect air shower observations of cosmic rays from 100 TeV to 1 EeV and gamma rays above 10 TeV to several PeV. In this paper the HiSCORE detector is discribed and the results of the first prototype deployment are shown. Several components are discussed like the photomultiplier tubes, the clip-sum-trigger and the DRS4 based data acquisition. We present data taken with a first prototype station in April 2012 at Tunka.

Published
2013
Full Text
View/download PDF

Catalog

Books, media, physical & digital resources
See catalog results