Radio emission of energetic cosmic ray air showers: Polarization measurements with LOPES

被引:13
|
作者
Isar, P. G. [1 ]
Apel, W. D. [1 ]
Arteaga, J. C. [2 ]
Asch, T. [3 ]
Auffenberg, J. [4 ]
Badea, F. [1 ]
Bahren, L. [5 ]
Bekk, K. [1 ]
Bertaina, M. [6 ]
Biermann, P. L. [7 ]
Bluemer, J. [1 ,2 ]
Bozdog, H. [1 ]
Brancus, I. M. [8 ]
Brueggemann, M. [9 ]
Buchholz, P. [9 ]
Buitink, S. [5 ]
Cantoni, E. [6 ,10 ]
Chiavassa, A. [6 ]
Cossavella, F. [2 ]
Daumiller, K. [1 ]
de Souza, V. [2 ]
Di Pierro, F. [6 ]
Doll, P. [1 ]
Engel, R. [1 ]
Falcke, H. [5 ,11 ]
Finger, M. [1 ]
Fuhrmann, D. [4 ]
Gemmeke, H. [3 ]
Ghia, P. L. [10 ]
Glasstetter, R. [4 ]
Grupen, C. [9 ]
Haungs, A. [1 ]
Heck, D. [1 ]
Horandel, J. R. [5 ]
Horneffer, A. [5 ]
Huang, X. [1 ]
Huege, T. [1 ]
Kampert, K. -H. [4 ]
Kang, D. [2 ]
Kickelbick, D. [9 ]
Kolotaev, Y. [9 ]
Kroemer, O. [3 ]
Kuijpers, J. [5 ]
Lafebre, S. [5 ]
Luczak, P. [12 ]
Mathes, H. J. [1 ]
Mayer, H. J. [1 ]
Milke, J. [1 ]
Mitrica, B. [8 ]
Morello, C. [10 ]
机构
[1] Forschungszentrum Karlsruhe, Inst Kernphys, Karlsruhe, Germany
[2] Univ Karlsruhe, Inst Expt Kernphys, Karlsruhe, Germany
[3] Forschungszentrum Karlsruhe, Inst Prozessdatenverarbeitung & Elekt, Karlsruhe, Germany
[4] Univ Wuppertal, Fachbereich Phys, Wuppertal, Germany
[5] Radboud Univ Nijmegen, Dept Astrophys, Nijmegen, Netherlands
[6] Gen Univ Torino, Dipartimento Fis, Turin, Italy
[7] Max Planck Inst Radioastron, D-5300 Bonn, Germany
[8] Natl Inst Phys & Nucl Engn, Bucharest, Romania
[9] Univ Siegen, Fachbereich Phys, D-57068 Siegen, Germany
[10] INAF, Ist Fis Spazio Interplanetario, Turin, Italy
[11] ASTRON, Dwingeloo, Netherlands
[12] Soltan Inst Nucl Studies, Lodz, Poland
[13] Univ Bucharest, Dept Phys, Bucharest, Romania
关键词
Cosmic ray air showers; Radio emission; Polarization characteristics;
D O I
10.1016/j.nima.2009.03.118
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
LOPES is a radio antenna array co-located with the Karlsruhe Shower Core and Array DEtector, KASCADE-Grande in Forschungszentrum Karlsruhe, Germany, which provides well-calibrated trigger information and air shower parameters for primary energies up to 10(18) eV. By the end of 2006, the radio antennas were re-configured to perform polarization measurements of the radio signal of cosmic ray air showers, recording in the same time both, the East-West and North-South polarization directions of the radio emission. The main goal of these measurements is to reconstruct the polarization characteristics of the emitted signal, This will allow a detailed comparison with theoretical predictions. The current status of these measurements is reported here. (C) 2009 Elsevier B.V. All rights reserved.
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页码:S81 / S84
页数:4
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