The AMY (Air Microwave Yield) experiment to measure the GHz emission from air shower plasma
J. Alvarez-Muniz, M. Blanco, M. Bohacova, B. Buonomo, G. Cataldi, M., R. Coluccia, P. Creti, I. De Mitri, C. Di Giulio, P. Facal San Luis, L., Foggetta, R. Gaior, D. Garcia-Fernandez, M. Iarlori, S. Le Coz, A., Letessier-Selvon, K. Louedec, I. C. Maris, D. Martello

TL;DR
The AMY experiment investigates GHz emission from air-shower plasma induced by electron beams, revealing that beam time structure significantly affects emission intensity, complicating extrapolation to atmospheric showers.
Contribution
This study provides new experimental data on molecular bremsstrahlung radiation from air showers and highlights the impact of beam time structure on emission measurements.
Findings
Emission intensity is strongly influenced by beam time structure
First measurements of GHz emission from air-shower plasma
Challenges in extrapolating laboratory results to atmospheric conditions
Abstract
The aim of the Air Microwave Yield (AMY) experiment is to investigate the Molecular Bremsstrahlung Radiation (MBR) emitted from an electron beam induced air-shower. The measurements have been performed with a 510 MeV electron beam at the Beam Test Facility (BTF) of Frascati INFN National Laboratories in a wide frequency range between 1 and 20 GHz. We present the experimental apparatus and the first results of the measurements. Contrary to what have been reported in a previous similar experiment~\cite{Gorham-SLAC}, we have found that the intensity of the emission is strongly influenced by the particular time structure of the accelerator beam. This makes very difficult the interpretation of the emission process and a realistic extrapolation of the emission yield to the plasma generated during the development of an atmospheric shower.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology · Dark Matter and Cosmic Phenomena
