منابع مشابه
Radio detection of cosmic ray air showers with LOPES
Radio detection of cosmic ray air showers with LOPES T. Huege, W.D. Apel, T. Asch, A.F. Badea, L. Bähren, K. Bekk, A. Bercuci, M. Bertaina, P.L. Biermann , J. Blümer, H. Bozdog, I.M. Brancus, S. Buitink, M. Brüggemann, P. Buchholz, H. Butcher, A. Chiavassa, F. Cossavella, K. Daumiller, F. Di Pierro, P. Doll, R. Engel, H. Falcke, H. Gemmeke, P.L. Ghia, R. Glasstetter, C. Grupen, A. Hakenjos, A. ...
متن کامل30TH INTERNATIONAL COSMIC RAY CONFERENCE Trigger Strategy for Radio Detection of Atmospheric Air Showers with LOPES
In the framework of LOPES (LOFAR PrototypE Station), a Self-Triggered Array of Radio detectors (STAR) is developed. The challenge of LOPES is to provide an independent self-trigger on radio emission of extensive air showers with primary energies above 5 · 10 eV. Measurements are done with an external trigger and self-trigger in radio loud and quiet areas. Based on these data the self-trigger is...
متن کاملLOPES Detecting Radio Emission from Cosmic Ray Air Showers
Radio pulses emitted in the atmosphere during the air shower development of high-energy primary cosmic rays were measured during the late 1960ies in the frequency range from 2 MHz to 520 MHz. Mainly due to difficulties with radio interference these measurements ceased in the late 1970ies. LOFAR (Low Frequency Array) is a new digital radio interferometer under development. Using high bandwidth A...
متن کاملRadio Detection of Cosmic Rays with LOPES ( LOPES Collaboration )
C. Grupen,1 W.D. Apel,2 T. Asch,3 A.F.Badea,2, 4 L. Bähren,5 K. Bekk,2 A. Bercuci,6 M. Bertaina,7 P.L. Biermann,8 J. Blümer,2, 9 H. Bozdog,2 I.M. Brancus,6 S. Buitink,10 M. Brüggemann,1 P. Buchholz,1 H. Butcher,5 A. Chiavassa,7 F. Cossavella,9 K. Daumiller,2 F. Di Pierro,7 P. Doll,2 R. Engel,2 H. Falcke,5, 8, 10 H. Gemmeke,3 P.L. Ghia,11 R. Glasstetter,12 A. Haungs,2 D. Heck,2 J.R. Hörandel,9 A...
متن کاملCosmic Ray Results from the IceTop Air Shower Array
IceTop, the surface component of the IceCube neutrino telescope at the South Pole, is an air-shower array which will finally consist of 160 ice Cherenkov tanks at 80 stations spread over an area of 1 km. Currently 40 stations are deployed and taking data. The detector is designed to cover the energy range above the knee up to about 10 eV and study the mass composition of primary cosmic rays. In...
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ژورنال
عنوان ژورنال: Nuclear Physics B - Proceedings Supplements
سال: 2008
ISSN: 0920-5632
DOI: 10.1016/j.nuclphysbps.2007.11.003