New measurements of cosmic ray air showers with the digital radio interferometer LOPES
Autor: | P. Łuczak, H. Gemmeke, N. Palmieri, M. Finger, Claus Grupen, A. Chiavassa, J. Wochele, Octavian Sima, M. Ludwig, D. Kang, D. Heck, H. Bozdog, S.J. Lafebre, Heino Falcke, J. Blümer, H. J. Mathes, Tim Huege, L. Bähren, A. Weindl, F.G. Schröder, O. Krömer, Jan Kuijpers, D. Huber, J. A. Zensus, E. Cantoni, Ralph Engel, M. Wommer, Alexandra Saftoiu, J.C. Arteaga, A. Schmidt, A. Horneffer, K. Bekk, C. Rühle, C. Morello, T. Asch, D. Fuhrmann, W. D. Apel, Peter L. Biermann, Markus Roth, J. Rautenberg, Peter Buchholz, G. Toma, T. Pierog, I.M. Brancus, S. Nehls, Kai Daumiller, V. de Souza, Jörg R. Hörandel, P.G. Isar, G.C. Trinchero, J. Oehlschläger, M. E. Bertaina, Stijn Buitink, K. Link, A. Haungs, H. Rebel, J. Zabierowski, H. Schieler, M. Melissas, P. Doll, K. H. Kampert |
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Rok vydání: | 2011 |
Předmět: |
Physics
Physics and Astronomy (miscellaneous) LOPES Frequency band Astrophysics::High Energy Astrophysical Phenomena Astronomy Astrophysics::Instrumentation and Methods for Astrophysics Astronomy and Astrophysics Cosmic ray Aetiology screening and detection [ONCOL 5] Astrophysics::Cosmology and Extragalactic Astrophysics Digital radio law.invention Radio telescope Interferometry Air shower law RÁDIO Dipole antenna GeneralLiterature_REFERENCE(e.g. dictionaries encyclopedias glossaries) |
Zdroj: | Astrophysics and Space Sciences Transactions (Astra), 7, 3, pp. 303-306 Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) Universidade de São Paulo (USP) instacron:USP Astrophysics and Space Sciences Transactions (Astra), 7, 303-306 |
ISSN: | 1810-6536 |
DOI: | 10.5194/astra-7-303-2011 |
Popis: | LOPES is a digital radio interferometer which measures the radio emission of extensive cosmic ray air showers. It mainly consists of 30 dipole antennas installed in co-location with KASCADE-Grande at the Karlsruhe Insti- tute of Technology (KIT) in Germany. KASCADE-Grande measures the secondary air shower particles at ground. Whenever KASCADE-Grande detects a high-energy cosmic ray event (� 10 16 eV), it triggers LOPES which then digi- tally records the radio signal in the frequency band from 40 to 80 MHz. Using interferometric methods, LOPES is able to successfully detect air shower induced radio pulses, even in the noisy environment at the KIT. In the present studies, a considerable progress in understanding the radio emission mechanism is shown: The latest version of the "radio emis |
Databáze: | OpenAIRE |
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