Towards real-time cosmic-ray identification with the LOw Frequency ARay

Towards real-time cosmic-ray identification with the LOw Frequency ARay

Antonio, Bonardi;Stijn, Buitink;Arthur, Corstanje;Heino, Falcke;M., Hare Brian;R., Hörandel Jörg;Pragati, Mitra;Katie, Mulrey;Anna, Nelles;P., Rachen Jörg;Laura, Rossetto;Pim, Schellart;Olaf, Scholten;Satyendra, Thoudam;T.N., Trinh Gia;Sander, ter Veen;Tobias, Winchen;
epj web of conferences 2019 Vol. 216 pp. 04005-
134
antonio2019towardsepj

Abstract

The radio signals emitted by Extensive Air Showers have been successfully used for the last decade by LOFAR to reconstruct the properties of the primary cosmic rays. Since an effective real-time recognition system for the very short radio pulses is lacking, cosmic-ray acquisition is currently triggered by an external array of particle detector, called LORA, limiting the LOFAR collecting area to the area covered by LORA. A new algorithm for the real-time cosmic-ray detection has been developed for the LOFAR Low Band Antenna, which are sensitive between 10 and 90 MHz, and is here presented together with the latest results.

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