Adelaide Research & Scholarship
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https://hdl.handle.net/2440/83082
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Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Berezhnev, S. | - |
| dc.contributor.author | Rowell, G. | - |
| dc.date.issued | 2013 | - |
| dc.identifier.citation | Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors, and Associated Equipment, 2013; 732:281-285 | - |
| dc.identifier.issn | 0168-9002 | - |
| dc.identifier.issn | 1872-9576 | - |
| dc.identifier.uri | http://hdl.handle.net/2440/83082 | - |
| dc.description.abstract | The EAS Cherenkov array Tunka-133, with about 3 km2 sensitive area, has been installed in the Tunka Valley, Siberia. The accessible energy range is 1015-1018 eV. In this contribution, a description of the array and main results obtained so far are presented. A current update of the array includes the deployment of scintillation stations, radio antennas, as well as optical stations. The deployments of these optical stations are the first step towards Tunka-HiSCORE, a wide-angle, large field-of-view gamma-ray telescope. © 2013 Elsevier B.V. | - |
| dc.description.statementofresponsibility | S.F. Berezhnev...G.P. Rowell...et al. | - |
| dc.language.iso | en | - |
| dc.publisher | Elsevier Science BV | - |
| dc.rights | © 2013 Elsevier B.V. All rights reserved. | - |
| dc.source.uri | http://dx.doi.org/10.1016/j.nima.2013.05.180 | - |
| dc.subject | Cosmic rays | - |
| dc.subject | Tunka-133 | - |
| dc.subject | Tunka-HiSCORE | - |
| dc.title | The Tunka - Multi-component EAS detector for high energy cosmic ray studies | - |
| dc.type | Journal article | - |
| dc.identifier.doi | 10.1016/j.nima.2013.05.180 | - |
| pubs.publication-status | Published | - |
| dc.identifier.orcid | Rowell, G. [0000-0002-9516-1581] | - |
| Appears in Collections: | Aurora harvest IPAS publications | |
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