Study of high energy cosmic rays with the sparse very large air shower array ALTA/CZELTA
- NázevTitle
- Study of high energy cosmic rays with the sparse very large air shower array ALTA/CZELTAStudy of high energy cosmic rays with the sparse very large air shower array ALTA/CZELTA
- Druh výsledkuResult type
- Příspěvek ve sborníkuProceedings paper
- AutořiAuthors
- K. Smolek, J. Čermák, S. Pospíšil, P. Přidal, J. Smejkal, I. Štekl, F. Blaschke, P. Lichard, J. Pinfold, R. Soluk, V. Vícha
- Klíčová slovaKeywords
- ALTA, CZELTA, large area array, cosmic ray, detector system
- KonferenceConference
- 11th ICATPP Conference on Astroparticle, Particle, Space Physics, Detectors and Medical Physics Applications (Villa Olmo, Italy, 2009-10-05)
- DOIDOI
- 10.1142/9789814307529_0127
- Časopis / citaceJournal / citation
- In: Astroparticle, Particle and Space Physics, Detectors and Medical Physics Applications, WORLD SCIENTIFIC, 2010, pp. 800-806
- RokYear
- 2010
- JazykLanguage
- eng
- ZáznamyRecords
- ProjektProject
- Fundamentální experimenty ve fyzice mikrosvětaFundamental Experiments in Physics of Microworld; Centrum experimentální jaderné astrofyziky a jaderné fyzikyCenter of Experimental Nuclear Astrophysics and Nuclear Physics
- Citace ke staženíDownload citation
- TXT · BibTeX
AbstraktAbstract
ALTA/CZELTA is the sparse network of stations for the detection of cosmic rays with energy more than 1014 eV. At present, the detector system covers large area in Canada (Alberta Large area Time coincidence Array) and in the Czech Republic (CZEch Large are Time coincidence Array). The network is designed to study of non-random component of cosmic rays over large distances. We present the design of the project and the first results of the analysis of measured data.
ALTA/CZELTA is the sparse network of stations for the detection of cosmic rays with energy more than 1014 eV. At present, the detector system covers large area in Canada (Alberta Large area Time coincidence Array) and in the Czech Republic (CZEch Large are Time coincidence Array). The network is designed to study of non-random component of cosmic rays over large distances. We present the design of the project and the first results of the analysis of measured data.