Tunka-133 EAS Cherenkov Array: Status of 2007

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dc.creatorBudnev, N. M.
dc.creatorChvalaev, O. V.
dc.creatorGress, O. A.
dc.creatorKalmykov, N. N.
dc.creatorKozhin, V. A.
dc.creatorKorosteleva, E. E.
dc.creatorKuzmichev, L. A.
dc.creatorLubsandorzhiev, B. K.
dc.creatorMirgazov, R. R.
dc.creatorNavarra, G.
dc.creatorPanasyuk, M. I.
dc.creatorPankov, L. V.
dc.creatorProsin, V. V.
dc.creatorPtuskin, V. S.
dc.creatorSemeney, Y. A.
dc.creatorSkurikhin, A. V.
dc.creatorShaibonov, B. A.
dc.creatorSpiering, Ch.
dc.creatorWieschnewski, R.
dc.creatorYashin, I. V.
dc.creatorZablotsky, A. V.
dc.creatorZagorodnikov, A. V.
dc.date2008-01-19
dc.date.accessioned2026-07-07T08:55:32Z
dc.date.available2026-07-07T08:55:32Z
dc.descriptionThe new EAS Cherenkov array Tunka-133, with about 1 km**2 sensitive area, is being installed in the Tunka Valley since the end of 2005. This array will permit a detailed study of the cosmic ray energy spectrum and the mass composition in the energy range of 10**15-10**18 eV with a unique method. The array will consist of 19 clusters, each composed of 7 optical detectors. The first cluster started operation in October 2006. We describe the data acquisition system and present preliminary results from data taken with the first cluster.
dc.description4 pages, 4 figures, Proceedings of 30th ICRC, Merinda, Mexico, July 2007
dc.identifierhttps://arxiv.org/abs/0801.3037
dc.identifierhttp://arxiv.org/abs/0801.3037
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/146299
dc.subjectAstrophysics
dc.titleTunka-133 EAS Cherenkov Array: Status of 2007
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