Experimental evidence for the sensitivity of the air-shower radio signal to the longitudinal shower development
arXiv:1203.3971 · doi:10.1103/PhysRevD.85.071101
Abstract
We observe a correlation between the slope of radio lateral distributions, and the mean muon pseudorapidity of 59 individual cosmic-ray-air-shower events. The radio lateral distributions are measured with LOPES, a digital radio interferometer co-located with the multi-detector-air-shower array KASCADE-Grande, which includes a muon-tracking detector. The result proves experimentally that radio measurements are sensitive to the longitudinal development of cosmic-ray air-showers. This is one of the main prerequisites for using radio arrays for ultra-high-energy particle physics and astrophysics.
6 pages, 5 figures, accepted for publication by Physical Review D
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- A comparison of the cosmic-ray energy scales of Tunka-133 and KASCADE-Grande via their radio extensions Tunka-Rex and LOPES
- The wavefront of the radio signal emitted by cosmic ray air showers
- First Experimental Characterization of Microwave Emission from Cosmic Ray Air Showers
- Final results of the LOPES radio interferometer for cosmic-ray air showers
- High-Energy Galactic Cosmic Rays (Astro2020 Science White Paper)
- Design and Expected Performance of the IceCube-Gen2 Surface Array and its Radio Component (ARENA2022)
- Radio Detection of ultra-high-energy Cosmic-Ray Air Showers
- Proof of principle for template synthesis approach for the radio emission from vertical extensive air showers
- Tunka-Rex: Status, Plans, and Recent Results (ARENA 2016)
- Status of air-shower measurements with sparse radio arrays (ARENA 2016)