Radio detection of cosmic rays with LOPES (LOPES Collaboration)
Autor(a) principal: | |
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Data de Publicação: | 2006 |
Outros Autores: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Brazilian Journal of Physics |
Texto Completo: | http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332006000700008 |
Resumo: | 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. |
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Radio detection of cosmic rays with LOPES (LOPES Collaboration)Cosmic raysExtensive air showerRadio emissionData 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.Sociedade Brasileira de Física2006-12-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersiontext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332006000700008Brazilian Journal of Physics v.36 n.4a 2006reponame:Brazilian Journal of Physicsinstname:Sociedade Brasileira de Física (SBF)instacron:SBF10.1590/S0103-97332006000700008info:eu-repo/semantics/openAccessGrupen,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.Di Pierro,F.Doll,P.Engel,R.Falcke,H.Gemmeke,H.Ghia,P.L.Glasstetter,R.Haungs,A.Heck,D.Hörandel,J.R.Horneffer,A.Huege,T.Kampert,K.H.Kolotaev,Y.Krömer,O.Kuijpers,J.Lafebre,S.Mathes,H.J.Mayer,H.J.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.Roth,M.Schieler,H.Sima,O.Singh,K.Stümpert,M.Toma,G.Trinchero,G.C.Ulrich,H.van Buren,J.Walkowiak,W.Weindl,A.Wochele,J.Zabierowski,J.Zensus,J.A.Zimmermann,D.eng2007-06-21T00:00:00Zoai:scielo:S0103-97332006000700008Revistahttp://www.sbfisica.org.br/v1/home/index.php/pt/ONGhttps://old.scielo.br/oai/scielo-oai.phpsbfisica@sbfisica.org.br||sbfisica@sbfisica.org.br1678-44480103-9733opendoar:2007-06-21T00:00Brazilian Journal of Physics - Sociedade Brasileira de Física (SBF)false |
dc.title.none.fl_str_mv |
Radio detection of cosmic rays with LOPES (LOPES Collaboration) |
title |
Radio detection of cosmic rays with LOPES (LOPES Collaboration) |
spellingShingle |
Radio detection of cosmic rays with LOPES (LOPES Collaboration) Grupen,C. Cosmic rays Extensive air shower Radio emission |
title_short |
Radio detection of cosmic rays with LOPES (LOPES Collaboration) |
title_full |
Radio detection of cosmic rays with LOPES (LOPES Collaboration) |
title_fullStr |
Radio detection of cosmic rays with LOPES (LOPES Collaboration) |
title_full_unstemmed |
Radio detection of cosmic rays with LOPES (LOPES Collaboration) |
title_sort |
Radio detection of cosmic rays with LOPES (LOPES Collaboration) |
author |
Grupen,C. |
author_facet |
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. Di Pierro,F. Doll,P. Engel,R. Falcke,H. Gemmeke,H. Ghia,P.L. Glasstetter,R. Haungs,A. Heck,D. Hörandel,J.R. Horneffer,A. Huege,T. Kampert,K.H. Kolotaev,Y. Krömer,O. Kuijpers,J. Lafebre,S. Mathes,H.J. Mayer,H.J. 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. Roth,M. Schieler,H. Sima,O. Singh,K. Stümpert,M. Toma,G. Trinchero,G.C. Ulrich,H. van Buren,J. Walkowiak,W. Weindl,A. Wochele,J. Zabierowski,J. Zensus,J.A. Zimmermann,D. |
author_role |
author |
author2 |
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. Di Pierro,F. Doll,P. Engel,R. Falcke,H. Gemmeke,H. Ghia,P.L. Glasstetter,R. Haungs,A. Heck,D. Hörandel,J.R. Horneffer,A. Huege,T. Kampert,K.H. Kolotaev,Y. Krömer,O. Kuijpers,J. Lafebre,S. Mathes,H.J. Mayer,H.J. 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. Roth,M. Schieler,H. Sima,O. Singh,K. Stümpert,M. Toma,G. Trinchero,G.C. Ulrich,H. van Buren,J. Walkowiak,W. Weindl,A. Wochele,J. Zabierowski,J. Zensus,J.A. Zimmermann,D. |
author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
dc.contributor.author.fl_str_mv |
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. Di Pierro,F. Doll,P. Engel,R. Falcke,H. Gemmeke,H. Ghia,P.L. Glasstetter,R. Haungs,A. Heck,D. Hörandel,J.R. Horneffer,A. Huege,T. Kampert,K.H. Kolotaev,Y. Krömer,O. Kuijpers,J. Lafebre,S. Mathes,H.J. Mayer,H.J. 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. Roth,M. Schieler,H. Sima,O. Singh,K. Stümpert,M. Toma,G. Trinchero,G.C. Ulrich,H. van Buren,J. Walkowiak,W. Weindl,A. Wochele,J. Zabierowski,J. Zensus,J.A. Zimmermann,D. |
dc.subject.por.fl_str_mv |
Cosmic rays Extensive air shower Radio emission |
topic |
Cosmic rays Extensive air shower Radio emission |
description |
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. |
publishDate |
2006 |
dc.date.none.fl_str_mv |
2006-12-01 |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332006000700008 |
url |
http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332006000700008 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
10.1590/S0103-97332006000700008 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
text/html |
dc.publisher.none.fl_str_mv |
Sociedade Brasileira de Física |
publisher.none.fl_str_mv |
Sociedade Brasileira de Física |
dc.source.none.fl_str_mv |
Brazilian Journal of Physics v.36 n.4a 2006 reponame:Brazilian Journal of Physics instname:Sociedade Brasileira de Física (SBF) instacron:SBF |
instname_str |
Sociedade Brasileira de Física (SBF) |
instacron_str |
SBF |
institution |
SBF |
reponame_str |
Brazilian Journal of Physics |
collection |
Brazilian Journal of Physics |
repository.name.fl_str_mv |
Brazilian Journal of Physics - Sociedade Brasileira de Física (SBF) |
repository.mail.fl_str_mv |
sbfisica@sbfisica.org.br||sbfisica@sbfisica.org.br |
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1754734863418654720 |