First Upper Limits on the Radar Cross Section of Cosmic-Ray Induced Extensive Air Showers
R.U. Abbasi, M. Abe, M. Abou Bakr Othman, T.Abu-Zayyad, M. Allen, R., Anderson, R. Azuma, E. Barcikowski, J.W. Belz, D.R. Bergman, D. Besson, S.A., Blake, M. Byrne, R. Cady, M.J. Chae, B.G. Cheon, J. Chiba, M. Chikawa, W.R., Cho, B. Farhang-Boroujeny, T. Fujii, M. Fukushima

TL;DR
This paper reports the first upper limits on the radar cross section of cosmic-ray induced air showers using the TARA radar detection experiment, which combines radar transmission with fluorescence detection to search for radar echoes.
Contribution
The study introduces a novel matched filter technique to search for radar echoes from air showers and provides the first quantitative upper limits on their radar cross section.
Findings
No evidence of radar scattering from air showers was detected.
Established upper limits on the radar cross section of extensive air showers.
Demonstrated the effectiveness of the matched filter search method.
Abstract
TARA (Telescope Array Radar) is a cosmic ray radar detection experiment colocated with Telescope Array, the conventional surface scintillation detector (SD) and fluorescence telescope detector (FD) near Delta, Utah, U.S.A. The TARA detector combines a 40 kW, 54.1 MHz VHF transmitter and high-gain transmitting antenna which broadcasts the radar carrier over the SD array and within the FD field of view, towards a 250 MS/s DAQ receiver. TARA has been collecting data since 2013 with the primary goal of observing the radar signatures of extensive air showers (EAS). Simulations indicate that echoes are expected to be short in duration (~10 microseconds) and exhibit rapidly changing frequency, with rates on the order of 1 MHz/microsecond. The EAS radar cross-section (RCS) is currently unknown although it is the subject of over 70 years of speculation. A novel signal search technique is…
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