Radiodetection of Cosmic Ray Extensive Air Showers

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dc.creatorArdouin, D.
dc.creatorBelletoile, A.
dc.creatorCharrier, D.
dc.creatorDallier, R.
dc.creatorDenis, L.
dc.creatorEschstruth, P.
dc.creatorGousset, T.
dc.creatorHaddad, F.
dc.creatorLamblin, J.
dc.creatorLautridou, P.
dc.creatorLecacheux, A.
dc.creatorMonnier-Ragaiggne, D.
dc.creatorRahmani, A.
dc.creatorRavel, O.
dc.creatorCollaboration, the Codalema
dc.date2004-12-09
dc.date.accessioned2026-07-07T06:26:01Z
dc.date.available2026-07-07T06:26:01Z
dc.descriptionWe present the characteristics and performance of a demonstration experiment devoted to the observation of ultra high- energy cosmic ray extensive air showers using a radiodetection technique. In a first step, one antenna narrowed band filtered acting as trigger, with a 4 $σ$ threshold above sky background-level, was used to tag any radio transient in coincidence on the antenna array. Recently, the addition of 4 particle detectors has allowed us to observe cosmic ray events in coincidence with antennas.
dc.identifierhttps://arxiv.org/abs/astro-ph/0412211
dc.identifierhttp://arxiv.org/abs/astro-ph/0412211
dc.identifierInt.J.Mod.Phys. A20 (2005) 6869-6871
dc.identifierdoi:10.1142/S0217751X0503034X
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/96993
dc.subjectAstrophysics
dc.titleRadiodetection of Cosmic Ray Extensive Air Showers
dc.typetext

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