Issue |
EPJ Web Conf.
Volume 135, 2017
7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities (ARENA 2016)
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|
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Article Number | 01017 | |
Number of page(s) | 4 | |
Section | Radio Detection of Extensive Air Showers | |
DOI | https://doi.org/10.1051/epjconf/201713501017 | |
Published online | 15 March 2017 |
https://doi.org/10.1051/epjconf/201713501017
SLAC T-510: Radio emission from particle cascades in the presence of a magnetic field
Vrije Universiteit Brussel
* e-mail: kmulrey@gmail.com
Published online: 15 March 2017
Cosmic ray induced particle cascades radiate in radio frequencies in the Earth’s atmosphere. Geomagnetic and Askaryan emission provide an effective way to detect ultra-high energy cosmic rays. The SLAC T-510 experiment was the first to measure magnetically induced radiation from particle cascades in a controlled laboratory setting. An electron beam incident upon a dense dielectric target produced a particle cascade in the presence of a variable magnetic field. Antennas covering a band of 30-3000 MHz sampled RF emission in vertical and horizontal polarizations. Results from T-510 are compared to particle-level RF-emission simulations which are critical for reconstructing the energy and composition of detected ultra-high energy cosmic ray air showers. We discuss the experimental set up, the data processing, the systematic errors and the main results of the experiment, which we found in a good agreement with the simulations.
© The Authors, published by EDP Sciences, 2017
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