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

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

2002-05-03

arxiv.org/abs/astro-ph/0205046v4

Nucl.Instrum.Meth. A498 (2003) 256-288

Astronomy and Astrophysics

Astrophysics

53 pages, LaTeX, 19 figures, published in Nuclear Instruments and Methods. Revised version; some references updated

Scientific paper

10.1016/S0168-9002(02)01995-2

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 hours of running time), taken under low-noise conditions, permitted upper limits to be placed on the rate for pulses accompanying showers of energies around $10^{17}$ eV.

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