LOPES-3D: An antenna array for full signal detection of air-shower radio emission

被引:16
作者
Apel, W. D. [2 ]
Arteaga, J. C. [1 ]
Bahren, L. [3 ]
Bekk, K. [2 ]
Bertaina, M. [4 ]
Biermann, P. L. [5 ]
Bluemer, J. [1 ,2 ]
Bozdog, H. [2 ]
Brancus, I. M. [6 ]
Buchholz, P. [7 ]
Cantoni, E. [4 ,8 ]
Chiavassa, A. [4 ]
Daumiller, K. [2 ]
de Souza, V. [1 ]
Di Pierro, F. [4 ]
Doll, P. [2 ]
Engel, R. [2 ]
Falcke, H. [3 ,5 ,9 ]
Finger, M. [1 ]
Fuchs, B. [1 ]
Fuhrmann, D. [10 ]
Gemmeke, H. [11 ]
Grupen, C. [7 ]
Haungs, A. [2 ]
Heck, D. [2 ]
Horandel, J. R. [3 ]
Horneffer, A. [5 ]
Huber, D. [1 ]
Huege, T. [2 ]
Isar, P. G. [2 ,14 ]
Kampert, K. -H. [10 ]
Kang, D. [1 ]
Kroemer, O. [11 ]
Kuijpers, J. [3 ]
Link, K. [1 ]
Luczak, P. [12 ]
Ludwig, M. [1 ]
Mathes, H. J. [2 ]
Melissas, M. [1 ]
Morello, C. [8 ]
Oehlschlaeger, J. [2 ]
Palmieri, N. [1 ]
Pierog, T. [2 ]
Rautenberg, J. [10 ]
Rebel, H. [2 ]
Roth, M. [2 ]
Ruehle, C. [11 ]
Saftoiu, A. [6 ]
Schieler, H. [2 ]
Schmidt, A. [11 ]
机构
[1] KIT, Inst Expt Kernphys, Karlsruhe, Germany
[2] KIT, Inst Kernphys, Karlsruhe, Germany
[3] Radboud Univ Nijmegen, Dept Astrophys, Nijmegen, Netherlands
[4] Univ Turin, Dipartimento Fis Gen, I-10124 Turin, Italy
[5] Max Planck Inst Radioastron Bonn, Bonn, Germany
[6] Natl Inst Phys & Nucl Engn, Bucharest, Romania
[7] Univ Siegen, Fachbereich Phys, D-57068 Siegen, Germany
[8] INAF Torino, Inst Fis Spazio Interplanetario, Taipei, Taiwan
[9] ASTRON, Dwingeloo, Netherlands
[10] Berg Univ Wuppertal, Fachbereich Phys, D-42097 Wuppertal, Germany
[11] KIT, Inst Prozessdatenverarbeitung & Elekt, Karlsruhe, Germany
[12] Natl Ctr Nucl Res, Dept Cosm Ray Phys, Lodz, Poland
[13] Univ Bucharest, Dept Phys, Bucharest, Romania
[14] Inst Space Sci, Bucharest, Romania
关键词
Cosmic rays; Extensive air showers; Electromagnetic radiation from moving charges; Radio detection; Full E-field vector; LOPES; COSMIC-RAYS; CALIBRATION;
D O I
10.1016/j.nima.2012.08.082
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
To better understand the radio signal emitted by extensive air-showers and to further develop the radio detection technique of high-energy cosmic rays, the LOPES experiment was reconfigured to LOPES-3D. LOPES-3D is able to measure all three vectorial components of the electric field of radio emission from cosmic ray air showers. The additional measurement of the vertical component ought to increase the reconstruction accuracy of primary cosmic ray parameters like direction and energy, provides an improved sensitivity to inclined showers, and will help to validate simulation of the emission mechanisms in the atmosphere. LOPES-3D will evaluate the feasibility of vectorial measurements for large scale applications. In order to measure all three electric field components directly, a tailor-made antenna type (tripoles) was deployed. The change of the antenna type necessitated new pre-amplifiers and an overall recalibration. The reconfiguration and the recalibration procedure are presented and the operationality of LOPES-3D is demonstrated. (C) 2012 Elsevier B.V. All rights reserved.
引用
收藏
页码:100 / 109
页数:10
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