Search

Your search keyword '"A.V. Zablotsky"' showing total 3 results
Start Over Author "A.V. Zablotsky" Language undetermined
3 results on '"A.V. Zablotsky"'

1. 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

2. 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

3. 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

Catalog

Books, media, physical & digital resources
See catalog results