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Radioelectric field features of extensive air showers observed with CODALEMA

2006/08/18 by D. Ardouin, A. Belletoile, A. Bellétoile +17 · 96 citations
Physics and Astronomy · #Air shower #Astrophysics #Astrophysics and Cosmic Phenomena #Computational physics #Cosmic ray #Dark Matter and Cosmic Phenomena #Electric field #Electrical engineering #Energy (signal processing) #Event (particle physics) #Field (mathematics) #Nuclear physics #Physics #Radio Astronomy Observations and Technology #Radio frequency #Radio signal #SIGNAL (programming language) #astro-ph

paper · pdf · doi:10.1016/j.astropartphys.2006.07.002

published in Astroparticle Physics 26(4-5), 341-350 (Elsevier BV) · Accepted for publication in Astroparticle Physics

openalex publication_date 2006/08/18 · arxiv created 2006/08/25 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Based on a new approach to the detection of radio transients associated with extensive air showers induced by ultra high energy cosmic rays, the experimental apparatus CODALEMA is in operation, measuring about 1 event per day corresponding to an energy threshold ~ 5. 1016 eV. Its performance makes possible for the first time the study of radio-signal features on an event-by-event basis. The sampling of the magnitude of the electric field along a 600 meters axis is analyzed. It shows that the electric field lateral spread is around 250 m (FWHM). The possibility to determine with radio both arrival directions and shower core positions is discussed.

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