Evidence for Radio Detection of Extensive Air Showers Induced by Ultra High Energy Cosmic Rays

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dc.creatorArdouin, D.
dc.creatorBellétoile, A.
dc.creatorCharrier, D.
dc.creatorDallier, R.
dc.creatorGousset, T.
dc.creatorHaddad, F.
dc.creatorLamblin, J.
dc.creatorLautridou, P.
dc.creatorRavel, O.
dc.creatorLecacheux, A.
dc.creatorDenis, L.
dc.creatorEschstruth, P.
dc.creatorMonnier-Ragaigne, D.
dc.date2005-04-11
dc.date.accessioned2026-07-07T02:17:26Z
dc.date.available2026-07-07T02:17:26Z
dc.descriptionFirm evidence for a radio emission counterpart of cosmic ray air showers is presented. By the use of an antenna array set up in coincidence with ground particle detectors, we find a collection of events for which both time and arrival direction coincidences between particle and radio signals are observed. The counting rate corresponds to shower energies $\gtrsim 5\times 10^{16}$ eV. These results open overwhelming perspectives to complete existing detection methods for the observation of ultra high-energy cosmic rays.
dc.description4 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0504240
dc.identifierhttp://arxiv.org/abs/astro-ph/0504240
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9169
dc.subjectAstrophysics
dc.titleEvidence for Radio Detection of Extensive Air Showers Induced by Ultra High Energy Cosmic Rays
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