Radio detection of cosmic rays with LOPES

C. Grupen; 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; A. Haungs; D. Heck; J. R. Hörandel; A. Horneffer; T. Huege; K. H. Kampert; Y. Kolotaev; O. Krömer; J. Kuijpers; S. Lafebre; H. J. Mathes; H. J. Mayer; C. Meurer; J. Milke; B. Mitrica; C. Morello; G. Navarra; S. Nehls; A. Nigl; R. Obenland; J. Oehlschläger; S. Ostapchenko; S. Over; M. Petcu; J. Petrovic; T. Pierog; S. Plewnia; H. Rebel; A. Risse; M. Roth; H. Schieler; O. Sima; K. Singh; M. Stümpert; G. Toma; G. C. Trinchero; H. Ulrich; J. Van Buren; W. Walkowiak; A. Weindl; J. Wochele; J. Zabierowski; J. A. Zensus; D. Zimmermann

doi:10.1590/S0103-97332006000700008

Radio detection of cosmic rays with LOPES

C. Grupen^*, 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 PierroP. Doll, R. Engel, H. Falcke, H. Gemmeke, P. L. Ghia, R. Glasstetter, A. Haungs, D. Heck, J. R. Hörandel, A. Horneffer, T. Huege, K. H. Kampert, Y. Kolotaev, O. Krömer, J. Kuijpers, S. Lafebre, H. J. Mathes, H. J. Mayer, C. Meurer, J. Milke, B. Mitrica, C. Morello, G. Navarra, S. Nehls, A. Nigl, R. Obenland, J. Oehlschläger, S. Ostapchenko, S. Over, M. Petcu, J. Petrovic, T. Pierog, S. Plewnia, H. Rebel, A. Risse, M. Roth, H. Schieler, O. Sima, K. Singh, M. Stümpert, G. Toma, G. C. Trinchero, H. Ulrich, J. Van Buren, W. Walkowiak, A. Weindl, J. Wochele, J. Zabierowski, J. A. Zensus, D. Zimmermann

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

2 Citations (Scopus)

Abstract

Data taken with a radio antenna array in combination with the ground-level air shower experiment KASCADE-Grande at the Forschungszentrum Karlsruhe open up the possibility to measure large extensive air showers with this new technique. The pulse height of the observed radio signals scales with the primary energy of the particles initiating the air shower. The dependence of the radio signal on the angle of the shower axis with respect to the Earth's geomagnetic field and the coherence of the radiation suggest that the radio signal generation is due to the geosynchrotron mechanism.

Original language	English
Pages (from-to)	1157-1164
Number of pages	8
Journal	Brazilian Journal of Physics
Volume	36
Issue number	4 A
DOIs	https://doi.org/10.1590/S0103-97332006000700008
Publication status	Published - Dec 2006
Externally published	Yes

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10.1590/S0103-97332006000700008

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Grupen, C., Apel, W. D., Asch, T., Badea, A. F., Bähren, L., Bekk, K., Bercuci, A., Bertaina, M., Biermann, P. L., Blümer, J., Bozdog, H., Brancus, I. M., Buitink, S., Brüggemann, M., Buchholz, P., Butcher, H., Chiavassa, A., Cossavella, F., Daumiller, K., ... Zimmermann, D. (2006). Radio detection of cosmic rays with LOPES. Brazilian Journal of Physics, 36(4 A), 1157-1164. https://doi.org/10.1590/S0103-97332006000700008

@article{8891c8e3ed34495e9b1e539fb11f5f6e,

title = "Radio detection of cosmic rays with LOPES",

abstract = "Data taken with a radio antenna array in combination with the ground-level air shower experiment KASCADE-Grande at the Forschungszentrum Karlsruhe open up the possibility to measure large extensive air showers with this new technique. The pulse height of the observed radio signals scales with the primary energy of the particles initiating the air shower. The dependence of the radio signal on the angle of the shower axis with respect to the Earth's geomagnetic field and the coherence of the radiation suggest that the radio signal generation is due to the geosynchrotron mechanism.",

keywords = "Cosmic rays, Extensive air shower, Radio emission",

author = "C. Grupen and Apel, {W. D.} and T. Asch and Badea, {A. F.} and L. B{\"a}hren and K. Bekk and A. Bercuci and M. Bertaina and Biermann, {P. L.} and J. Bl{\"u}mer and H. Bozdog and Brancus, {I. M.} and S. Buitink and M. Br{\"u}ggemann and P. Buchholz and H. Butcher and A. Chiavassa and F. Cossavella and K. Daumiller and {Di Pierro}, F. and P. Doll and R. Engel and H. Falcke and H. Gemmeke and Ghia, {P. L.} and R. Glasstetter and A. Haungs and D. Heck and H{\"o}randel, {J. R.} and A. Horneffer and T. Huege and Kampert, {K. H.} and Y. Kolotaev and O. Kr{\"o}mer and J. Kuijpers and S. Lafebre and Mathes, {H. J.} and Mayer, {H. J.} and C. Meurer and J. Milke and B. Mitrica and C. Morello and G. Navarra and S. Nehls and A. Nigl and R. Obenland and J. Oehlschl{\"a}ger and S. Ostapchenko and S. Over and M. Petcu and J. Petrovic and T. Pierog and S. Plewnia and H. Rebel and A. Risse and M. Roth and H. Schieler and O. Sima and K. Singh and M. St{\"u}mpert and G. Toma and Trinchero, {G. C.} and H. Ulrich and {Van Buren}, J. and W. Walkowiak and A. Weindl and J. Wochele and J. Zabierowski and Zensus, {J. A.} and D. Zimmermann",

year = "2006",

month = dec,

doi = "10.1590/S0103-97332006000700008",

language = "English",

volume = "36",

pages = "1157--1164",

journal = "Brazilian Journal of Physics",

issn = "0103-9733",

publisher = "Springer",

number = "4 A",

}

Grupen, C, Apel, WD, Asch, T, Badea, AF, Bähren, L, Bekk, K, Bercuci, A, Bertaina, M, Biermann, PL, Blümer, J, Bozdog, H, Brancus, IM, Buitink, S, Brüggemann, M, Buchholz, P, Butcher, H, Chiavassa, A, Cossavella, F, Daumiller, K, Di Pierro, F, Doll, P, Engel, R, Falcke, H, Gemmeke, H, Ghia, PL, Glasstetter, R, Haungs, A, Heck, D, Hörandel, JR, Horneffer, A, Huege, T, Kampert, KH, Kolotaev, Y, Krömer, O, Kuijpers, J, Lafebre, S, Mathes, HJ, Mayer, HJ, Meurer, C, Milke, J, Mitrica, B, Morello, C, Navarra, G, Nehls, S, Nigl, A, Obenland, R, Oehlschläger, J, Ostapchenko, S, Over, S, Petcu, M, Petrovic, J, Pierog, T, Plewnia, S, Rebel, H, Risse, A, Roth, M, Schieler, H, Sima, O, Singh, K, Stümpert, M, Toma, G, Trinchero, GC, Ulrich, H, Van Buren, J, Walkowiak, W, Weindl, A, Wochele, J, Zabierowski, J, Zensus, JA & Zimmermann, D 2006, 'Radio detection of cosmic rays with LOPES', Brazilian Journal of Physics, vol. 36, no. 4 A, pp. 1157-1164. https://doi.org/10.1590/S0103-97332006000700008

TY - JOUR

T1 - Radio detection of cosmic rays with LOPES

AU - Grupen, C.

AU - Apel, W. D.

AU - Asch, T.

AU - Badea, A. F.

AU - Bähren, L.

AU - Bekk, K.

AU - Bercuci, A.

AU - Bertaina, M.

AU - Biermann, P. L.

AU - Blümer, J.

AU - Bozdog, H.

AU - Brancus, I. M.

AU - Buitink, S.

AU - Brüggemann, M.

AU - Buchholz, P.

AU - Butcher, H.

AU - Chiavassa, A.

AU - Cossavella, F.

AU - Daumiller, K.

AU - Di Pierro, F.

AU - Doll, P.

AU - Engel, R.

AU - Falcke, H.

AU - Gemmeke, H.

AU - Ghia, P. L.

AU - Glasstetter, R.

AU - Haungs, A.

AU - Heck, D.

AU - Hörandel, J. R.

AU - Horneffer, A.

AU - Huege, T.

AU - Kampert, K. H.

AU - Kolotaev, Y.

AU - Krömer, O.

AU - Kuijpers, J.

AU - Lafebre, S.

AU - Mathes, H. J.

AU - Mayer, H. J.

AU - Meurer, C.

AU - Milke, J.

AU - Mitrica, B.

AU - Morello, C.

AU - Navarra, G.

AU - Nehls, S.

AU - Nigl, A.

AU - Obenland, R.

AU - Oehlschläger, J.

AU - Ostapchenko, S.

AU - Over, S.

AU - Petcu, M.

AU - Petrovic, J.

AU - Pierog, T.

AU - Plewnia, S.

AU - Rebel, H.

AU - Risse, A.

AU - Roth, M.

AU - Schieler, H.

AU - Sima, O.

AU - Singh, K.

AU - Stümpert, M.

AU - Toma, G.

AU - Trinchero, G. C.

AU - Ulrich, H.

AU - Van Buren, J.

AU - Walkowiak, W.

AU - Weindl, A.

AU - Wochele, J.

AU - Zabierowski, J.

AU - Zensus, J. A.

AU - Zimmermann, D.

PY - 2006/12

Y1 - 2006/12

N2 - Data taken with a radio antenna array in combination with the ground-level air shower experiment KASCADE-Grande at the Forschungszentrum Karlsruhe open up the possibility to measure large extensive air showers with this new technique. The pulse height of the observed radio signals scales with the primary energy of the particles initiating the air shower. The dependence of the radio signal on the angle of the shower axis with respect to the Earth's geomagnetic field and the coherence of the radiation suggest that the radio signal generation is due to the geosynchrotron mechanism.

AB - Data taken with a radio antenna array in combination with the ground-level air shower experiment KASCADE-Grande at the Forschungszentrum Karlsruhe open up the possibility to measure large extensive air showers with this new technique. The pulse height of the observed radio signals scales with the primary energy of the particles initiating the air shower. The dependence of the radio signal on the angle of the shower axis with respect to the Earth's geomagnetic field and the coherence of the radiation suggest that the radio signal generation is due to the geosynchrotron mechanism.

KW - Cosmic rays

KW - Extensive air shower

KW - Radio emission

UR - http://www.scopus.com/inward/record.url?scp=34248345001&partnerID=8YFLogxK

U2 - 10.1590/S0103-97332006000700008

DO - 10.1590/S0103-97332006000700008

M3 - Article

SN - 0103-9733

VL - 36

SP - 1157

EP - 1164

JO - Brazilian Journal of Physics

JF - Brazilian Journal of Physics

IS - 4 A

ER -

Radio detection of cosmic rays with LOPES

Abstract

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