Geomagnetic origin of the radio emission from cosmic ray induced air showers observed by CODALEMA
The new setup of the CODALEMA experiment installed at the Radio Observatory in Nançay, France, is described. It includes broadband active dipole antennas and an extended and upgraded particle detector array.

Published by D. Ardouin, A. Bellétoile, C. Berat, D. Breton, D. Charrier, J. Chauvin, M. Chendeb, A. Cordier, S. Dagoret-Campagne, R. Dallier, L. Denis, C. Dumez-Viou, C. Fabrice, T. Garçon, X. Garrido, N. Gautherot, T. Gousset, F. Haddad, D.H. Koang, J. Lamblin, P. Lautridou, D. Lebrun, A. Lecacheux, F. Lefeuvre, L. Martin, E. Meyer, F. Meyer, N. Meyer-Vernet, D. Monnier-Ragaigne, F. Montanet, K. Payet G. Plantier, O. Ravel, B. Revenu, C. Riviere, T. Saugrin, A. Sourice, P. Stassi, A. Stutz, S. Valcares, in Astroparticle Physics 31, January 2009, P. 192–200 https://doi.org/10.1016/j.astropartphys.2009.01.001