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On noise treatment in radio measurements of cosmic ray air showers

✍ Scribed by F.G. Schröder; W.D. Apel; J.C. Arteaga; T. Asch; L. Bähren; K. Bekk; M. Bertaina; P.L. Biermann; J. Blümer; H. Bozdog; I.M. Brancus; P. Buchholz; S. Buitink; E. Cantoni; A. Chiavassa; K. Daumiller; V. de Souza; P. Doll; R. Engel; H. Falcke; M. Finger; D. Fuhrmann; H. Gemmeke; C. Grupen; A. Haungs; D. Heck; J.R. Hörandel; A. Horneffer; D. Huber; T. Huege; P.G. Isar; K.-H. Kampert; D. Kang; O. Krömer; J. Kuijpers; S. Lafebre; K. Link; P. łuczak; M. Ludwig; H.J. Mathes; M. Melissas; C. Morello; S. Nehls; J. Oehlschläger; N. Palmieri; T. Pierog; J. Rautenberg; H. Rebel; M. Roth; C. Rühle; A. Saftoiu; H. Schieler; A. Schmidt; O. Sima; G. Toma; G.C. Trinchero; A. Weindl; J. Wochele; M. Wommer; J. Zabierowski; J.A. Zensus

Book ID
113821701
Publisher
Elsevier Science
Year
2012
Tongue
English
Weight
315 KB
Volume
662
Category
Article
ISSN
0168-9002

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In the last few years, radio detection of cosmic ray air showers has experienced a true renaissance, becoming manifest in a number of new experiments and simulation efforts. In particular, the LOPES project has successfully implemented modern interferometric methods to measure the radio emission fro