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Your search keyword '"R.R. Mirgazov"' showing total 7 results
Start Over Author "R.R. Mirgazov" Publisher elsevier bv
7 results on '"R.R. Mirgazov"'

1. Tunka-133: Results of 3 year operation

Author

V.V. Prosin, S.F. Berezhnev, N.M. Budnev, A. Chiavassa, O.A. Chvalaev, O.A. 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, M.I. Panasyuk, L.V. Pan'kov, E.G. Popova, V.S. Ptuskin, Yu.A. Semeney, A.A. Silaev, A.V. Skurikhin, C. Spiering, L.G. Sveshnikova, I.V. Yashin, and A.V. Zagorodnikov

Subjects
Physics, Nuclear and High Energy Physics, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, Astrophysics, Mass composition, Electromagnetic radiation, Spectral line, Computational physics, Data acquisition, Range (statistics), ddc:530, Instrumentation, Energy (signal processing), Cherenkov radiation
Abstract

The EAS Cherenkov light array Tunka-133, with ~3 km2 geometric area, is taking data since 2009. The array permits a detailed study of cosmic ray energy spectrum and mass composition in the PeV energy range. After a short description of the methods of EAS parameter reconstruction, we present the all-particle energy spectrum and results of studying CR composition, based on 3 seasons of array operation. In the last part of the paper, we discuss possible interpretations of the obtained results.

Published
2014
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2. The Tunka – Multi-component EAS detector for high energy cosmic ray studies

Author

S.F. Berezhnev, D. Besson, N.M. Budnev, M. Büker, M. Brüeckner, A. Chiavassa, O.A. Chvalaev, O.A. Gress, A.N. Dyachok, S.N. Epimakhov, D. Hampf, A. Haungs, R. Hiller, D. Horns, A. Ivanova, N.I. Karpov, N.N. Kalmykov, Yu. Kazarina, E.N. Konstantinov, D. Kostunin, A.V. Korobchenko, E.E. Korosteleva, V.A. Kozhin, M. Kunnas, L.A. Kuzmichev, B.K. Lubsandorzhiev, N.B. Lubsandorzhiev, R.R. Mirgazov, R. Monhoev, R. Nachtigall, M.I. Panasyuk, L.V. Pankov, A.L. Pankov, A. Pokhorukov, E.G. Popova, A. Porelli, V.V. Prosin, V.S. Ptuskin, G.P. Rowell, F.G. Schröder, Yu.A. Semeney, B.A. Shaibonov, A.A. Silaev, A.V. Skurikhin, C. Spiering, D. Spitschan, L.G. Sveshnikova, R. Wischnewski, I.V. Yashin, and A.V. Zagorodnikov

Subjects
Physics, Nuclear and High Energy Physics, Scintillation, High energy, Range (particle radiation), Detector, Astronomy, Cosmic ray, law.invention, Telescope, law, Instrumentation, Cherenkov radiation, Energy (signal processing), Remote sensing
Abstract

The EAS Cherenkov array Tunka-133, with about 3 km 2 sensitive area, has been installed in the Tunka Valley, Siberia. The accessible energy range is 10 15 –10 18 eV. In this contribution, a description of the array and main results obtained so far are presented. A current update of the array includes the deployment of scintillation stations, radio antennas, as well as optical stations. The deployments of these optical stations are the first step towards Tunka-HiSCORE, a wide-angle, large field-of-view gamma-ray telescope.

Published
2013
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3. Tunka-133: preliminary results from the first year of operation

Author

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

Subjects
Physics, Nuclear and High Energy Physics, Optical detectors, COSMIC cancer database, Pulse waveform, Meteorology, ddc:530, Cosmic ray, Atomic and Molecular Physics, and Optics, Cherenkov radiation, Remote sensing
Abstract

The new array Tunka-133 started data taking at the end of 2009. The apparatus records the Cherenkov light pulse waveform of extensive air showers (EAS). It consists of 133 optical detectors deployed over an area of about 1 km 2 . About two million events have been collected during 286 hours of clean moonless nights in winter 2009-2010. Using these data, we present methods of primary cosmic particle parameter reconstruction for EAS with the core both inside and outside the array and give preliminary results.

Published
2011
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4. The new Tunka-133 EAS Cherenkov array: Status of 2009

Author

B.V. Antokhonov, S.F. Beregnev, N.M. Budnev, O.B. Chvalaev, A. Chiavassa, O.A. Gress, N.N. Kalmykov, N.N. Karpov, E.E. Korosteleva, V.A. Kozhin, L.A. Kuzmichev, B.K. Lubsandorzhiev, R.R. Mirgazov, M.I. Panasyuk, L.V. Pankov, V.V. Prosin, V.S. Ptuskin, Yu.A. Semeney, B. Shaibonov, A.A. Silaev, A.V. Skurikhin, Ch. Spiering, R. Wischnewski, I.V. Yashin, A.V. Zablotsky, and A.V. Zagorodnikov

Subjects
Physics, Nuclear and High Energy Physics, Cherenkov detector, Astronomy, Cosmic ray, Mass composition, law.invention, Data acquisition, Air shower, law, Energy spectrum, ddc:530, Instrumentation, Cherenkov radiation, Remote sensing
Abstract

The deployment of the new Extensive air shower Cherenkov installation Tunka-133 with about 1 km 2 geometric acceptance area was completed in October 2009. The array will permit a detailed long-term study of the cosmic ray energy spectrum and mass composition in the energy range 10 15 –10 18 eV with a unique and more elaborate method. The array construction and data acquisition system, preliminary results and plans for future development are presented.

Published
2011
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5. The Cosmic Ray Mass Composition in the Energy Range measured with the Tunka Array: Results and Perspectives

Author

V.V. Prosin, N.M. Budnev, O.A. Chvalaiev, O.A. Gress, N.N. Kalmykov, V.A. Kozhin, E.E. Korosteleva, L.A. Kuzmichev, B.K. Lubsandorzhiev, R.R. Mirgazov, G. Navarra, M.I. Panasyuk, L.V. Pankov, V.S. Ptuskin, Yu.A. Semeney, B.A. Shaibonov, A.A. Silaev, A.V. Skurikhin, C. Spiering, R. Wischnewski, I.V. Yashin, A.V. Zablotsky, and A.V. Zagorodnikov

Subjects
Nuclear physics, Physics, Nuclear and High Energy Physics, Range (particle radiation), Air shower, Cosmic ray, Mass composition, Atomic and Molecular Physics, and Optics, Cherenkov radiation, Energy (signal processing)
Abstract

The final analysis of the Extensive Air Shower (EAS) maximum ( X m a x ) depth distribution derived from the data of Tunka-25 atmospheric Cherenkov light array in the energy range 3 ⋅ 10 15 – 3 ⋅ 10 16 eV is presented. The perspectives of X m a x studies with the new Cherenkov light array Tunka-133 of 1 km 2 area, extending the measurements up to 10 18 eV, are discussed.

Published
2009
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6. Registration of atmospheric neutrinos with the BAIKAL Neutrino Telescope NT-96

Author

V.A. Balkanov, I.A. Belolaptikov, L.B. Bezrukov, N.M. Budnev, A.G. Chensky, I.A. Danilchenko, Zh.-A.M. Djilkibaev, G.V. Domogatsky, A.A. Doroshenko, S.V. Fialkovsky, O.N. Gaponenko, A.A. Garus, T.I. Gress, A.M. Klabukov, A.I. Klimov, S.I. Klimushin, A.P. Koshechkin, V.F. Kulepov, L.A. Kuzmichev, V.E. Kuznetzov, J.J. Laudinskaite, S.V. Lovtzov, B.K. Lubsandorzhiev, M.B. Milenin, R.R. Mirgazov, N.I. Moseiko, V.A. Netikov, E.A. Osipova, A.I. Panfilov, Yu.V. Parfenov, A.A. Pavlov, E.N. Pliskovsky, P.G. Pokhil, E.G. Popova, M.I. Rozanov, V.Yu. Rubtzov, I.A. Sokalski, Ch. Spiering, O. Streicher, B.A. Tarashansky, T. Thon, R.V. Vasiljev, R. Wischnewski, and I.V. Yashin

Subjects
Physics, Muon, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Monte Carlo method, Neutrino telescope, Flux, Astronomy and Astrophysics, Astrophysics, law.invention, Telescope, law, High Energy Physics::Experiment, Underwater, Neutrino, Zenith
Abstract

We present first neutrino induced events observed with a deep underwater neutrino telescope. Data from 70 days effective life time of the BAIKAL prototype telescope NT-96 have been analyzed with two different methods. With the standard track reconstruction method, 9 clear upward muon candidates have been identified, in good agreement with 8.7 events expected from Monte Carlo calculations for atmospheric neutrinos. The second analysis is tailored to muons coming from close to the opposite zenith. It yields 4 events, compared to 3.5 from Monte Carlo expectations. From this we derive a 90 % upper flux limit of 1.1 * 10^-13 cm^-2 sec^-1 for muons in excess of those expected from atmospheric neutrinos with zenith angle > 150 degrees and energy > 10GeV.

Published
1999
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7. Status of the AMANDA and BAIKAL neutrino telescopes

Author

P. Askebjer, S.W. Barwick, R. Bay, L. Bergström, A. Bouchta, S. Carius, E. Dahlberg, K. Engel, B. Erlandsson, A. Goobar, L. Gray, A. Hallgren, F. Halzen, H. Heukenkamp, P.O. Hulth, S. Hundertmark, J. Jacobsen, S. Johansson, V. Kandhadai, A. Karle, I. Liubarsky, D. Lowder, T. Mikolajski, T.C. Miller, P. Mock, R. Morse, D. Nygren, R. Porrata, P.B. Price, A. Richards, H. Rubinstein, E. Schneider, C. Spiering, O. Streicher, Q. Sun, T. Thon, S. Tilav, C. Walck, C. Wiebusch, R. Wischnewski, G. Yodh, I.A. Belolaptikov, L.B. Bezrukov, B.A. Borisovets, N.M. Budnev, A.G. Chensky, I.A. Danilchenko, Zh.-A.M. Djilkibaev, V.I. Dobrynin, G.V. Domogatsky, A.A. Doroshenko, S.V. Fialkovsky, O.N. Gaponenko, A.A. Garus, T.A. Gress, S.B. Ignat'ev, A.M. Klabukov, A.I. Klimov, S.I. Klimushin, A.P. Koshechkin, V.F. Kulepov, L.A. Kuzmichev, B.K. Lubsandorzhiev, M.B. Milenin, R.R. Mirgazov, A.V. Moroz, N.I. Moseiko, S.A. Nikiforov, E.A. Osipova, D. Pandel, A.I. Panfilov, Yu.V. Parfenov, A.A. Pavlov, D.P. Petukhov, K.A. Pocheikin, P.G. Pokhil, P.A. Pokolev, M.I. Rosanov, V.Yu. Rubzov, S.I. Sinegovsky, I.A. Sokalski, Ch. Spiering, and B.A. Tarashansky

Subjects
Astroparticle physics, Physics, Nuclear and High Energy Physics, Particle physics, Neutrino, Atomic and Molecular Physics, and Optics
Published
1997
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