On noise treatment in radio measurements of cosmic ray air showers

Abstract

Precise measurements of the radio emission by cosmic ray air showers require an adequate treatment of noise. Unlike to usual experiments in particle physics, where noise always adds to the signal, radio noise can in principle decrease or increase the signal if it interferes by chance destructively or constructively. Consequently, noise cannot simply be subtracted from the signal, and its influence on amplitude and time measurement of radio pulses must be studied with care. First, noise has to be determined consistently with the definition of the radio signal which typically is the maximum field strength of the radio pulse. Second, the average impact of noise on radio pulse measurements at individual antennas is studied for LOPES. It is shown that a correct treatment of noise is especially important at low signal-to-noise ratios: noise can be the dominant source of uncertainty for pulse height and time measurements, and it can systematically flatten the slope of lateral distributions. The presented method can also be transfered to other experiments in radio and acoustic detection of cosmic rays and neutrinos.

4 pages, 6 figures, submitted to NIM A, Proceedings of ARENA 2010, Nantes, France

References in corpus (3)

• Lateral Distribution of the Radio Signal in Extensive Air Showers Measured with LOPES
• New method for the time calibration of an interferometric radio antenna array
• Amplitude calibration of a digital radio antenna array for measuring cosmic ray air showers

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