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| 001 | 50033 | ||
| 005 | 20250129092403.0 | ||
| 024 | 7 | _ | |2 DOI |a 10.1016/j.nuclphysbps.2005.01.197 |
| 024 | 7 | _ | |2 WOS |a WOS:000228672500118 |
| 037 | _ | _ | |a PreJuSER-50033 |
| 041 | _ | _ | |a eng |
| 082 | _ | _ | |a 530 |
| 084 | _ | _ | |2 WoS |a Physics, Particles & Fields |
| 100 | 1 | _ | |a Bosetti, P. C. |b 0 |0 P:(DE-HGF)0 |
| 245 | _ | _ | |a A low budget detector for high energy cosmic ray experiments |
| 260 | _ | _ | |a Amsterdam |b Elsevier |c 2005 |
| 300 | _ | _ | |a 532 |
| 336 | 7 | _ | |a Journal Article |0 PUB:(DE-HGF)16 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a Output Types/Journal article |2 DataCite |
| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
| 336 | 7 | _ | |a JOURNAL_ARTICLE |2 ORCID |
| 336 | 7 | _ | |a article |2 DRIVER |
| 440 | _ | 0 | |a Nuclear Physics B Proceedings Supplements |x 0920-5632 |0 4648 |v 143 |
| 500 | _ | _ | |a Record converted from VDB: 12.11.2012 |
| 520 | _ | _ | |a Contemporary projects such as AUGER in Argentina or HESS in Namibia are rather expensive experiments. We have constructed a simple detector arrangernent based on the water Cherenkov technique to be used for the detection of high-energy particles in cosmic ray experiments either as stand-alone experiment or as addition to other set-ups. A first prototype has been taken into successful operation. The construction of this detector is the starting point for extended studies in future cosmic ray experiments. The detector can be expanded by adding more and more modules at a very low price. |
| 536 | _ | _ | |a Betrieb und Weiterentwicklung des Kühler-Synchrotrons COSY |c M04 |2 G:(DE-HGF) |0 G:(DE-Juel1)FUEK244 |x 0 |
| 588 | _ | _ | |a Dataset connected to Web of Science |
| 650 | _ | 7 | |a J |2 WoSType |
| 700 | 1 | _ | |a Braun, U. |b 1 |0 P:(DE-HGF)0 |
| 700 | 1 | _ | |a Ransoné, G. |b 2 |0 P:(DE-HGF)0 |
| 700 | 1 | _ | |a Rössler, O. E. |b 3 |0 P:(DE-HGF)0 |
| 700 | 1 | _ | |a Engels, R. |b 4 |u FZJ |0 P:(DE-Juel1)133882 |
| 700 | 1 | _ | |a Kemmerling, G. |b 5 |u FZJ |0 P:(DE-Juel1)VDB2183 |
| 700 | 1 | _ | |a Flyckt, S. O. |b 6 |0 P:(DE-HGF)0 |
| 700 | 1 | _ | |a Fontaine, C. |b 7 |0 P:(DE-HGF)0 |
| 700 | 1 | _ | |a Lavoute, P. |b 8 |0 P:(DE-HGF)0 |
| 700 | 1 | _ | |a Marmonier, C. |b 9 |0 P:(DE-HGF)0 |
| 773 | _ | _ | |a 10.1016/j.nuclphysbps.2005.01.197 |g Vol. 143, p. 532 |p 532 |q 143<532 |0 PERI:(DE-600)1466572-4 |t Nuclear physics |v 143 |y 2005 |x 0920-5632 |
| 856 | 7 | _ | |u http://dx.doi.org/10.1016/j.nuclphysbps.2005.01.197 |
| 909 | C | O | |o oai:juser.fz-juelich.de:50033 |p VDB |
| 913 | 1 | _ | |k M04 |v Betrieb und Weiterentwicklung des Kühler-Synchrotrons COSY |l Kernphysik |b Materie |0 G:(DE-Juel1)FUEK244 |x 0 |
| 914 | 1 | _ | |y 2005 |
| 915 | _ | _ | |0 StatID:(DE-HGF)0010 |a JCR/ISI refereed |
| 920 | 1 | _ | |k ZEL |l Zentralinstitut für Elektronik |g ZEL |0 I:(DE-Juel1)ZEL-20090406 |x 0 |
| 970 | _ | _ | |a VDB:(DE-Juel1)78230 |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a ConvertedRecord |
| 980 | _ | _ | |a journal |
| 980 | _ | _ | |a I:(DE-Juel1)ZEA-2-20090406 |
| 980 | _ | _ | |a UNRESTRICTED |
| 981 | _ | _ | |a I:(DE-Juel1)PGI-4-20110106 |
| 981 | _ | _ | |a I:(DE-Juel1)ZEA-2-20090406 |
| 981 | _ | _ | |a I:(DE-Juel1)ZEL-20090406 |
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