Radioelectric Field Features of Extensive Air Showers Observed with CODALEMA
| dc.creator | Ardouin, D. | |
| dc.creator | Belletoile, A. | |
| dc.creator | Charrier, D. | |
| dc.creator | Dallier, R. | |
| dc.creator | Denis, L. | |
| dc.creator | Eschstruth, P. | |
| dc.creator | Gousset, T. | |
| dc.creator | Haddad, F. | |
| dc.creator | Lamblin, J. | |
| dc.creator | Lautridou, P. | |
| dc.creator | Lecacheux, A. | |
| dc.creator | Monnier-Ragaigne, D. | |
| dc.creator | Ravel, O. | |
| dc.creator | Saugrin, T. | |
| dc.creator | Valcares, S. | |
| dc.date | 2006-08-25 | |
| dc.date.accessioned | 2026-07-07T10:39:52Z | |
| dc.date.available | 2026-07-07T10:39:52Z | |
| dc.description | 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. 10^16 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. | |
| dc.description | Accepted for publication in Astroparticle Physics | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0608550 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0608550 | |
| dc.identifier | Astropart.Phys.26:341-350,2006 | |
| dc.identifier | doi:10.1016/j.astropartphys.2006.07.002 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/181180 | |
| dc.subject | Astrophysics | |
| dc.title | Radioelectric Field Features of Extensive Air Showers Observed with CODALEMA | |
| dc.type | text |