First upper limits on the radar cross section of cosmic-ray induced extensive air showers
- Univ. of Utah, Salt Lake City, UT (United States)
- Saitama Univ. (Japan)
- Tokyo Inst. of Technology (Japan)
- Univ. of Kansas, Lawrence, KS (United States); Moscow Engineering Physics Univ., Moscow (Russian Federation)
- Ewha Womans Univ., Seoul (Korea)
- Hanyang Univ., Seoul (Korea)
- Tokyo Univ. of Science, Chiba (Japan)
- Kinki Univ., Osaka (Japan)
- Yonsei Univ., Seoul (Korea)
- Univ. of Tokyo, Chiba (Japan)
- Univ. of Tokyo (Japan); Univ. of Tokyo, Chiba (Japan). Kavli Inst. for the Physics and Mathematics of the Universe (WPI)
- Gillman and Associates, Salt Lake City, UT (United States)
- Osaka City Univ. (Japan)
- Univ. of Kansas, Lawrence, KS (United States)
- Kanagawa Univ. (Japan)
- Univ. of Yamanashi (Japan)
- RIKEN, Saitama (Japan)
- Tokyo City Univ. (Japan)
- National Nuclear Research Univ., Moscow (Russia)
- Waseda Univ., Shinjuku (Japan)
- Chiba Univ. (Japan)
- Univ. of Tokyo, Chiba (Japan). Kavli Inst. for the Physics and Mathematics of the Universe (WPI)
- The High Energy Accelerator Research Organization (KEK) Ibaraki (Japan)
- Kochi Univ. (Japan)
- Ritsumeikan Univ., Shiga (Japan)
- Kyushu Univ. (Japan)
- Chuba Univ., Aichi (Japan)
- Sungkyunkwan Univ., Suwan (Korea)
- Moscow M.V.Lomonosov State Univ. (Russia); National Nuclear Research Univ., Moscow (Russia)
- Ulsan National Inst. of Science and Technology, Ulsan (Korea)
- Rutgers Univ., Piscataway, NJ (United States)
- Univ. of Utah, Salt Lake City, UT (United States); Rutgers Univ., Piscataway, NJ (United States)
- Brookhaven National Lab. (BNL), Upton, NY (United States)
- Univ. of Tokyo (Japan)
- High Energy Accelerator Research Organization (KEK), Tsukuba (Japan)
- National Nuclear Research Univ., Moscow (Russia); Free Univ. of Brussels (Belgium)
- Shinshu Univ., Nagano (Japan)
- National Inst. of Radiological Science, Chiba (Japan)
- Free Univ. of Brussels (Belgium)
- Ehime Univ., Matsuyama (Japan)
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. Furthermore, 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 µs) and exhibit rapidly changing frequency, with rates on the order 1 MHz/µs. The EAS radar cross-section (RCS) is currently unknown although it is the subject of over 70 years of speculation. One novel signal search technique is described in which the expected radar echo of a particular air shower is used as a matched filter template and compared to waveforms obtained by triggering the radar DAQ using the Telescope Array fluorescence detector. No evidence for the scattering of radio frequency radiation by EAS is obtained to date. Finally, we report the first quantitative RCS upper limits using EAS that triggered the Telescope Array Fluorescence Detector.
- Research Organization:
- Brookhaven National Laboratory (BNL), Upton, NY (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- Grant/Contract Number:
- SC00112704
- OSTI ID:
- 1377051
- Report Number(s):
- BNL-114194-2017-JA
- Journal Information:
- Astroparticle Physics, Vol. 87, Issue C; ISSN 0927-6505
- Publisher:
- ElsevierCopyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
Suggestion of coherent radio reflections from an electron-beam induced particle cascade
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journal | October 2019 |
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