EPJ Web Conf.
Volume 135, 20177th International Conference on Acoustic and Radio EeV Neutrino Detection Activities (ARENA 2016)
|Number of page(s)||4|
|Section||Radio Detection of Extensive Air Showers|
|Published online||15 March 2017|
Towards real-time identification of cosmic rays with LOw-Frequency ARray radio antennas
1 Department of Astrophysics/IMAPP, Radboud University, P.O. Box 9010, 6500 GL Nijmegen ( The Netherlands )
2 Vrije Universiteit Brussel, Pleinlaan 2, 1050 Brussels ( Belgium )
3 Astron, Oude Hoogeveensedijk 4, 7991 PD Dwingeloo ( The Netherlands )
4 Nikhef, Science Park 105, 1098 XG Amsterdam ( The Netherlands )
5 University of California Irvine, Irvine, CA 92697, ( USA )
6 KVI-CART, Zernikelaan 25, 9747 AA Groningen ( The Netherlands )
7 University of Groningen, Zernikelaan 25, 9747 AA Groningen ( The Netherlands )
* e-mail: firstname.lastname@example.org
Published online: 15 March 2017
Cosmic rays entering the Earth’s atmosphere produce Extensive Air Showers, which emit a radio signal through Geo-magnetic radiation and Askaryan emission. At the present time, one of the biggest challenges for assessing the Radio detection as a valuable technique for Cosmic-ray observation is to identify in real-time the very short (less than 100 ns) radio signals over the background noise. In this work, we present the latest updates on the real-time identification of radio signals from Extensive Air Showers by using the data from LOFAR Low Band Antenna stations, which are sensitive in the 30-80 MHz region.
© The Authors, published by EDP Sciences, 2017
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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