|
|||||
|
|
Tunka-133: Status 2008 and development of methods for data analysis |
|
| Authors: | N. M. Budnev R. Wishnevski O. A. Gress A. V. Zabolotsky A. V. Zagorodnikov N. N. Kalmykov V. A. Kozhin E. E. Korosteleva L. A. Kuzmichev B. K. Lubsandorzhiev G. Navarra R. R. Mirgazov M. I. Panasyuk L. V. Pankov V. V. Prosin V. S. Ptuskin Yu. A. Semeney A. A. Silaev A. A. Silaev Jr. A. V. Skurikhin O. A. Chvalaiev B. A. Shaibonov Ch. Spierin I. V. Yashin |
| Affiliation: | (1) Research Institute of Applied Physics, Irkutsk State University, Irkutsk, Russia;(2) DESY-Zeuthen, Zeuthen, Germany;(3) Skobel’tsyn Institute of Nuclear Physics, Moscow State University, Moscow, Russia;(4) Institute for Nuclear Research, Russian Academy of Sciences, Moscow, Russia;(5) University of Torino, Torino, Italy;(6) Institute of Terrestrial Magnetism, the Ionosphere, and the Radio-Wave Propagation, Russian Academy of Sciences, Troitsk, Moscow oblast, Russia |
| Abstract: | The activity on creation of a array with an area of 1 km2 for recording extensive air showers using Cherenkov light began in the Tunka valley in 2006. The new array will allow one to study cosmic rays in the energy range 1015–1018 eV by the unified method. In the winter of 2007–2008, the array operated with 4 clusters, 7 detectors in each cluster. Experimental data obtained during 270 h of fair weather in moonless nights demonstrated unique capabilities of the new array, related with the possibility of recording the pulse shape with a step of 5 ns from each detector. |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ | |