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27 April 2024
 
  » arxiv » 1308.2512

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Vectorial Radio Interferometry with LOPES 3D
D. Huber ; W.D. Apel ; J.C. Arteaga ; L. Bähren ; K. Bekk ; M. Bertaina ; P.L. Biermann ; J. Blümer ; H. Bozdog ; I.M. Brancus ; A. Chiavassa ; K. Daumiller ; V. de Souza ; F. Di Pierro ; P. Doll ; R. Engel ; H. Falcke ; B. Fuchs ; D. Fuhrmann ; H. Gemmeke ; C. Grupen ; A. Haungs ; D. Heck ; J.R. Hörandel ; A. Horneffer ; T. Huege ; P.G. Isar ; K.H. Kampert ; D. Kang ; O. Krömer ; J. Kuijpers ; K. Link ; P. Łuczak ; M. Ludwig ; H.J. Mathes ; M. Melissas ; C. Morello ; J. Oehlschläger ; N. Palmieri ; T. Pierog ; J. Rautenberg ; H. Rebel ; M. Roth ; C. Rühle ; A. Saftoiu ; H. Schieler ; A. Schmid ; F.G. Schröder ; O. Sima ; G. Toma ; G.C. Trinchero ; A. Weindl ; J. Wochele ; M. Wommer ; J. Zabierowski ; J.A. Zensus ;
Date 12 Aug 2013
AbstractOne successful detection technique for high-energy cosmic rays is based on the radio signal emitted by the charged particles in an air shower. The LOPES experiment at Karlsruhe Institute of Technology, Germany, has made major contributions to the evolution of this technique. LOPES was reconfigured several times to improve and further develop the radio detection technique. In the latest setup LOPES consisted of 10 tripole antennas. With this, LOPES 3D was the first cosmic ray experiment measuring all three vectorial field components at once and thereby gaining the full information about the electric field vector. We present an analysis based on the data taken with special focus on the benefits of a direct measurement of the vertical polarization component. We demonstrate that by measuring all polarization components the detection and reconstruction efficiency is increased and noisy single channel data can be reconstructed by utilising the information from the other two channels of one antenna station.
Source arXiv, 1308.2512
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