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Design of a low noise, wide band, active dipole antenna for a cosmic ray radiodetection experiment

Abstract : An active dipole antenna has been designed to measure transient electric field induced by ultra high energy cosmic rays for the CODALEMA experiment. The main requirements for this detector, composed of a low noise preamplifier placed close to a dipole antenna, are a wide bandwidth ranging from 100 kHz to 100 MHz and a good sensitivity on the whole spectrum.
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Submitted on : Friday, June 20, 2008 - 11:14:47 AM
Last modification on : Friday, June 22, 2018 - 9:34:48 AM

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Didier Charrier. Design of a low noise, wide band, active dipole antenna for a cosmic ray radiodetection experiment. Antennas and Propagation International Symposium, 2007 IEEE, Jun 2007, Honolulu, United States. pp.4485-4488, ⟨10.1109/APS.2007.4396539⟩. ⟨in2p3-00289282⟩

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