A prototype system for detecting the radio-frequency pulse associated with cosmic ray air showers

Abstract The development of a system to detect the radio-frequency (RF) pulse associated with extensive air showers of cosmic rays is described. This work was performed at the CASA/MIA array in Utah, with the intention of designing equipment that can be used in conjunction with the Auger Giant Array. A small subset of data (less than 40 out of a total of 600 h of running time), taken under low-noise conditions, permitted upper limits to be placed on the rate and strength of pulses accompanying showers with energies around 10 17 eV .