000050033 001__ 50033
000050033 005__ 20250129092403.0
000050033 0247_ $$2DOI$$a10.1016/j.nuclphysbps.2005.01.197
000050033 0247_ $$2WOS$$aWOS:000228672500118
000050033 037__ $$aPreJuSER-50033
000050033 041__ $$aeng
000050033 082__ $$a530
000050033 084__ $$2WoS$$aPhysics, Particles & Fields
000050033 1001_ $$0P:(DE-HGF)0$$aBosetti, P. C.$$b0
000050033 245__ $$aA low budget detector for high energy cosmic ray experiments
000050033 260__ $$aAmsterdam$$bElsevier$$c2005
000050033 300__ $$a532
000050033 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article
000050033 3367_ $$2DataCite$$aOutput Types/Journal article
000050033 3367_ $$00$$2EndNote$$aJournal Article
000050033 3367_ $$2BibTeX$$aARTICLE
000050033 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000050033 3367_ $$2DRIVER$$aarticle
000050033 440_0 $$04648$$aNuclear Physics B Proceedings Supplements$$v143$$x0920-5632
000050033 500__ $$aRecord converted from VDB: 12.11.2012
000050033 520__ $$aContemporary projects such as AUGER in Argentina or HESS in Namibia are rather expensive experiments. We have constructed a simple detector arrangernent based on the water Cherenkov technique to be used for the detection of high-energy particles in cosmic ray experiments either as stand-alone experiment or as addition to other set-ups. A first prototype has been taken into successful operation. The construction of this detector is the starting point for extended studies in future cosmic ray experiments. The detector can be expanded by adding more and more modules at a very low price.
000050033 536__ $$0G:(DE-Juel1)FUEK244$$2G:(DE-HGF)$$aBetrieb und Weiterentwicklung des Kühler-Synchrotrons COSY$$cM04$$x0
000050033 588__ $$aDataset connected to Web of Science
000050033 650_7 $$2WoSType$$aJ
000050033 7001_ $$0P:(DE-HGF)0$$aBraun, U.$$b1
000050033 7001_ $$0P:(DE-HGF)0$$aRansoné, G.$$b2
000050033 7001_ $$0P:(DE-HGF)0$$aRössler, O. E.$$b3
000050033 7001_ $$0P:(DE-Juel1)133882$$aEngels, R.$$b4$$uFZJ
000050033 7001_ $$0P:(DE-Juel1)VDB2183$$aKemmerling, G.$$b5$$uFZJ
000050033 7001_ $$0P:(DE-HGF)0$$aFlyckt, S. O.$$b6
000050033 7001_ $$0P:(DE-HGF)0$$aFontaine, C.$$b7
000050033 7001_ $$0P:(DE-HGF)0$$aLavoute, P.$$b8
000050033 7001_ $$0P:(DE-HGF)0$$aMarmonier, C.$$b9
000050033 773__ $$0PERI:(DE-600)1466572-4$$a10.1016/j.nuclphysbps.2005.01.197$$gVol. 143, p. 532$$p532$$q143<532$$tNuclear physics <Amsterdam> / B / Proceedings supplements$$v143$$x0920-5632$$y2005
000050033 8567_ $$uhttp://dx.doi.org/10.1016/j.nuclphysbps.2005.01.197
000050033 909CO $$ooai:juser.fz-juelich.de:50033$$pVDB
000050033 9131_ $$0G:(DE-Juel1)FUEK244$$bMaterie$$kM04$$lKernphysik$$vBetrieb und Weiterentwicklung des Kühler-Synchrotrons COSY$$x0
000050033 9141_ $$y2005
000050033 915__ $$0StatID:(DE-HGF)0010$$aJCR/ISI refereed
000050033 9201_ $$0I:(DE-Juel1)ZEL-20090406$$gZEL$$kZEL$$lZentralinstitut für Elektronik$$x0
000050033 970__ $$aVDB:(DE-Juel1)78230
000050033 980__ $$aVDB
000050033 980__ $$aConvertedRecord
000050033 980__ $$ajournal
000050033 980__ $$aI:(DE-Juel1)ZEA-2-20090406
000050033 980__ $$aUNRESTRICTED
000050033 981__ $$aI:(DE-Juel1)PGI-4-20110106
000050033 981__ $$aI:(DE-Juel1)ZEA-2-20090406
000050033 981__ $$aI:(DE-Juel1)ZEL-20090406