ÚTEFČVUT Ústav technické a experimentální fyziky ČVUT v PrazeInstitute of Experimental and Applied Physics, CTU in Prague

CZELTA: An overview of the CZECH large-area time coincidence array

NázevTitle
CZELTA: An overview of the CZECH large-area time coincidence arrayCZELTA: An overview of the CZECH large-area time coincidence array
Druh výsledkuResult type
Článek v časopiseJournal article
AutořiAuthors
F. Blaschke, J. Čermák, J. Hubík, P. Lichard, P. Přidal, J. Smejkal, K. Smolek, I. Štekl, V. Vícha
Klíčová slovaKeywords
ALTA, CZELTA, large area array, cosmic ray, detector system
KonferenceConference
22nd European Cosmic Ray Symposium (Turku, Finland, 2010-08-03)
DOIDOI
10.5194/astra-7-69-2011
Časopis / citaceJournal / citation
Astrophysics and Space Sciences Transactions 7(1), 69-73 (2011) · ISSN 1810-6528
RokYear
2011
JazykLanguage
eng
ZáznamyRecords
ProjektProject
Centrum experimentální jaderné astrofyziky a jaderné fyzikyCenter of Experimental Nuclear Astrophysics and Nuclear Physics; Fundamentální experimenty ve fyzice mikrosvětaFundamental Experiments in Physics of Microworld
CitovánoCited by
13 (INSPIRE-HEP)
2011: 12012: 12013: 02014: 02015: 02016: 02017: 12018: 22019: 22020: 22021: 32022: 1
Citace ke staženíDownload citation
TXT · BibTeX

AbstraktAbstract

Main goal of the project CZELTA (CZEch Large-area Time coincidence Array) is to study global properties of high-energetic cosmic rays. To present date, project consists of 5 stations covering large area in the Czech republic capable of detection of extensive air showers with energy exceeding 1014 eV. Such a network of distant stations can be an ideal tool for probing global structure of cosmic rays. We present the design of the detection system and obtained results.

Main goal of the project CZELTA (CZEch Large-area Time coincidence Array) is to study global properties of high-energetic cosmic rays. To present date, project consists of 5 stations covering large area in the Czech republic capable of detection of extensive air showers with energy exceeding 1014 eV. Such a network of distant stations can be an ideal tool for probing global structure of cosmic rays. We present the design of the detection system and obtained results.

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