Adelaide Research & Scholarship
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https://hdl.handle.net/2440/82899
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Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Kunnas, M. | - |
| dc.contributor.author | Rowell, G. | - |
| dc.date.issued | 2014 | - |
| dc.identifier.citation | Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors, and Associated Equipment, 2014; 742:269–270- | - |
| dc.identifier.issn | 0168-9002 | - |
| dc.identifier.issn | 1872-9576 | - |
| dc.identifier.uri | http://hdl.handle.net/2440/82899 | - |
| dc.description.abstract | As a non-imaging wide-angle Cherenkov air shower detector array with an area of up to 100 km2, the HiSCORE (Hundred?i Square km Cosmic ORigin Explorer) detector concept allows measurements of gamma rays and cosmic rays in an energy range of 10 TeV up to 1 EeV. In the framework of the Tunka-HiSCORE project we have started measurements with a small prototype array, and planned to build an engineering array (1 km2) on the site of the Tunka experiment in Siberia. The first results and the most important hardware components are presented here. © 2013 Elsevier B.V. | - |
| dc.description.statementofresponsibility | M. Kunnas … G.P. Rowell … et al. | - |
| dc.language.iso | en | - |
| dc.publisher | Elsevier | - |
| dc.rights | © 2013, Elsevier B.V. All rights reserved. | - |
| dc.source.uri | http://dx.doi.org/10.1016/j.nima.2013.12.025 | - |
| dc.subject | HiSCORE | - |
| dc.subject | Astroparticle | - |
| dc.subject | Non-imaging Cherenkov experiment | - |
| dc.title | Hardware and first results of TUNKA-HiSCORE | - |
| dc.type | Journal article | - |
| dc.contributor.organisation | Institute for Photonics & Advanced Sensing (IPAS) | - |
| dc.identifier.doi | 10.1016/j.nima.2013.12.025 | - |
| pubs.publication-status | Published | - |
| dc.identifier.orcid | Rowell, G. [0000-0002-9516-1581] | - |
| Appears in Collections: | Aurora harvest IPAS publications | |
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