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. Haungs; D. Heck; J. R. Hörandel; A. Horneffer; P. G. Isar; 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:10.1016/j.nuclphysbps.2006.11.046

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 PierroP. Doll, R. Engel, H. Falcke, H. Gemmeke, P. L. Ghia, R. Glasstetter, C. Grupen, A. Hakenjos, A. Haungs, D. Heck, J. R. Hörandel, A. Horneffer, P. G. Isar, 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

4 Citations (Scopus)

Abstract

In the last few years, radio detection of cosmic ray air showers has experienced a true renaissance, becoming manifest in a number of new experiments and simulation efforts. In particular, the LOPES project has successfully implemented modern interferometric methods to measure the radio emission from extensive air showers. LOPES has confirmed that the emission is coherent and of geomagnetic origin, as expected by the geosynchrotron mechanism, and has demonstrated that a large scale application of the radio technique has great potential to complement current measurements of ultra-high energy cosmic rays. We describe the current status, most recent results and open questions regarding radio detection of cosmic rays and give an overview of ongoing research and development for an application of the radio technique in the framework of the Pierre Auger Observatory.

Original language	English
Pages (from-to)	341-348
Number of pages	8
Journal	Nuclear Physics B - Proceedings Supplements
Volume	165
DOIs	https://doi.org/10.1016/j.nuclphysbps.2006.11.046
Publication status	Published - Mar 2007
Externally published	Yes

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10.1016/j.nuclphysbps.2006.11.046

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Huege, T., 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. (2007). Radio detection of cosmic ray air showers with LOPES. Nuclear Physics B - Proceedings Supplements, 165, 341-348. https://doi.org/10.1016/j.nuclphysbps.2006.11.046

@article{f661628f60c540b0af8f767a8a3eb04e,

title = "Radio detection of cosmic ray air showers with LOPES",

abstract = "In the last few years, radio detection of cosmic ray air showers has experienced a true renaissance, becoming manifest in a number of new experiments and simulation efforts. In particular, the LOPES project has successfully implemented modern interferometric methods to measure the radio emission from extensive air showers. LOPES has confirmed that the emission is coherent and of geomagnetic origin, as expected by the geosynchrotron mechanism, and has demonstrated that a large scale application of the radio technique has great potential to complement current measurements of ultra-high energy cosmic rays. We describe the current status, most recent results and open questions regarding radio detection of cosmic rays and give an overview of ongoing research and development for an application of the radio technique in the framework of the Pierre Auger Observatory.",

author = "T. Huege 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 C. Grupen and A. Hakenjos and A. Haungs and D. Heck and H{\"o}randel, {J. R.} and A. Horneffer and Isar, {P. G.} 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 = "2007",

month = mar,

doi = "10.1016/j.nuclphysbps.2006.11.046",

language = "English",

volume = "165",

pages = "341--348",

journal = "Nuclear Physics B - Proceedings Supplements",

issn = "0920-5632",

publisher = "Elsevier B.V.",

}

Huege, T, 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, Grupen, C, Hakenjos, A, Haungs, A, Heck, D, Hörandel, JR, Horneffer, A, Isar, PG, 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 2007, 'Radio detection of cosmic ray air showers with LOPES', Nuclear Physics B - Proceedings Supplements, vol. 165, pp. 341-348. https://doi.org/10.1016/j.nuclphysbps.2006.11.046

TY - JOUR

T1 - Radio detection of cosmic ray air showers with LOPES

AU - Huege, T.

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 - Grupen, C.

AU - Hakenjos, A.

AU - Haungs, A.

AU - Heck, D.

AU - Hörandel, J. R.

AU - Horneffer, A.

AU - Isar, P. G.

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 - 2007/3

Y1 - 2007/3

N2 - In the last few years, radio detection of cosmic ray air showers has experienced a true renaissance, becoming manifest in a number of new experiments and simulation efforts. In particular, the LOPES project has successfully implemented modern interferometric methods to measure the radio emission from extensive air showers. LOPES has confirmed that the emission is coherent and of geomagnetic origin, as expected by the geosynchrotron mechanism, and has demonstrated that a large scale application of the radio technique has great potential to complement current measurements of ultra-high energy cosmic rays. We describe the current status, most recent results and open questions regarding radio detection of cosmic rays and give an overview of ongoing research and development for an application of the radio technique in the framework of the Pierre Auger Observatory.

AB - In the last few years, radio detection of cosmic ray air showers has experienced a true renaissance, becoming manifest in a number of new experiments and simulation efforts. In particular, the LOPES project has successfully implemented modern interferometric methods to measure the radio emission from extensive air showers. LOPES has confirmed that the emission is coherent and of geomagnetic origin, as expected by the geosynchrotron mechanism, and has demonstrated that a large scale application of the radio technique has great potential to complement current measurements of ultra-high energy cosmic rays. We describe the current status, most recent results and open questions regarding radio detection of cosmic rays and give an overview of ongoing research and development for an application of the radio technique in the framework of the Pierre Auger Observatory.

UR - http://www.scopus.com/inward/record.url?scp=33846795912&partnerID=8YFLogxK

U2 - 10.1016/j.nuclphysbps.2006.11.046

DO - 10.1016/j.nuclphysbps.2006.11.046

M3 - Article

SN - 0920-5632

VL - 165

SP - 341

EP - 348

JO - Nuclear Physics B - Proceedings Supplements

JF - Nuclear Physics B - Proceedings Supplements

ER -

Radio detection of cosmic ray air showers with LOPES

Abstract

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