Event calendar file
- icrc2007@icrc2007.unam.mx
Support
Tunka-133 EAS Cherenkov Array: Status of 2007
Speakers
- Prof. Vasily PROSIN
Primary authors
- Prof. Vasily PROSIN (Scobeltsyn Institut of Nuclear Physics of MSU, Moscow, Russia)
Co-authors
- Nikolai BUDNEV (Institute of Applied Physics of ISU, Irkutsk, Russia)
- Gianni NAVARRA (Universita' Torino, Italy)
- Michael PANASYUK (Scobeltsyn Institut of Nuclear Physics of MSU, Moscow, Russia)
- Leonid PANKOV (Institute of Applied Physics of ISU, Irkutsk, Russia)
- Vladimir PTUSKIN (IZMIRAN, Moscow, Russia)
- Yury SEMENEY (Institute of Applied Physics of ISU, Irkutsk, Russia)
- Alexandr SKURIKHIN (Scobeltsyn Institut of Nuclear Physics of MSU, Moscow, Russia)
- Bator SHAIBONOV(JUNIOR) (Institute for Nuclear Research of RAS, Moscow, Russia)
- Christian SPIERING (DESY-Zeuthen, Zeuthen, Germany)
- Ralf WISCHNEWSKI (DESY-Zeuthen, Zeuthen, Germany)
- Ivan YASHIN (Scobeltsyn Institut of Nuclear Physics of MSU, Moscow, Russia)
- Oleg CHVALAEV (Institute of Applied Physics of ISU, Irkutsk, Russia)
- Alexey ZABLOTSKY (Scobeltsyn Institut of Nuclear Physics of MSU, Moscow, Russia)
- Alexey ZAGORODNIKOV (Institute of Applied Physics of ISU, Irkutsk, Russia)
- Oleg GRESS (Institute of Applied Physics of ISU, Irkutsk, Russia)
- Nikolai KALMYKOV (Scobeltsyn Institut of Nuclear Physics of MSU, Moscow, Russia)
- Vladimir KOZHIN (Scobeltsyn Institut of Nuclear Physics of MSU, Moscow, Russia)
- Elena KOROSTELEVA (Scobeltsyn Institut of Nuclear Physics of MSU, Moscow, Russia)
- Leonid KUZMICHEV (Scobeltsyn Institut of Nuclear Physics of MSU, Moscow, Russia)
- Baiarto LUBSANDORZHIEV (Institute for Nuclear Research of RAS, Moscow, Russia)
- Rashid MIRGAZOV (Institute of Applied Physics of ISU, Irkutsk, Russia)
Files
Abstract content
The new EAS Cherenkov array Tunka-133 of a sensitive area about 1 km^2 is mounting in Tunka valley since the end of 2005. The new array will permit a detailed study of cosmic ray energy spectrum and mass composition in the energy range 10^15 - 10^18 eV with the unique method. The array will consist of 19 clasters each containing 7 optical detectors. The first claster started operation since October 2006. We discribe the data aqcuisition system of the array and present the preliminaty results of the test operation.
If this papers is presented for a collaboration, please specify the collaboration
Tunka Collaboration
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 5 (HE part 2), pages 973-976
