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

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 trigge...

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Main Authors: Bonardi Antonio, Buitink Stijn, Corstanje Arthur, Falcke Heino, Hare Brian M., Hörandel Jörg R., Mitra Pragati, Mulrey Katie, Nelles Anna, Rachen Jörg P., Rossetto Laura, Schellart Pim, Scholten Olaf, Thoudam Satyendra, Trinh Gia T.N., ter Veen Sander, Winchen Tobias
Format: Article
Language:English
Published: EDP Sciences 2019-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2019/21/epjconf_arena2018_04005.pdf
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spelling doaj-0834a30858544aa48ba5b3209727c2572021-08-02T13:33:39ZengEDP SciencesEPJ Web of Conferences2100-014X2019-01-012160400510.1051/epjconf/201921604005epjconf_arena2018_04005Towards real-time cosmic-ray identification with the LOw Frequency ARayBonardi AntonioBuitink StijnCorstanje ArthurFalcke HeinoHare Brian M.Hörandel Jörg R.Mitra PragatiMulrey KatieNelles AnnaRachen Jörg P.Rossetto LauraSchellart PimScholten OlafThoudam SatyendraTrinh Gia T.N.ter Veen SanderWinchen TobiasThe 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.https://www.epj-conferences.org/articles/epjconf/pdf/2019/21/epjconf_arena2018_04005.pdf
collection DOAJ
language English
format Article
sources DOAJ
author Bonardi Antonio
Buitink Stijn
Corstanje Arthur
Falcke Heino
Hare Brian M.
Hörandel Jörg R.
Mitra Pragati
Mulrey Katie
Nelles Anna
Rachen Jörg P.
Rossetto Laura
Schellart Pim
Scholten Olaf
Thoudam Satyendra
Trinh Gia T.N.
ter Veen Sander
Winchen Tobias
spellingShingle Bonardi Antonio
Buitink Stijn
Corstanje Arthur
Falcke Heino
Hare Brian M.
Hörandel Jörg R.
Mitra Pragati
Mulrey Katie
Nelles Anna
Rachen Jörg P.
Rossetto Laura
Schellart Pim
Scholten Olaf
Thoudam Satyendra
Trinh Gia T.N.
ter Veen Sander
Winchen Tobias
Towards real-time cosmic-ray identification with the LOw Frequency ARay
EPJ Web of Conferences
author_facet Bonardi Antonio
Buitink Stijn
Corstanje Arthur
Falcke Heino
Hare Brian M.
Hörandel Jörg R.
Mitra Pragati
Mulrey Katie
Nelles Anna
Rachen Jörg P.
Rossetto Laura
Schellart Pim
Scholten Olaf
Thoudam Satyendra
Trinh Gia T.N.
ter Veen Sander
Winchen Tobias
author_sort Bonardi Antonio
title Towards real-time cosmic-ray identification with the LOw Frequency ARay
title_short Towards real-time cosmic-ray identification with the LOw Frequency ARay
title_full Towards real-time cosmic-ray identification with the LOw Frequency ARay
title_fullStr Towards real-time cosmic-ray identification with the LOw Frequency ARay
title_full_unstemmed Towards real-time cosmic-ray identification with the LOw Frequency ARay
title_sort towards real-time cosmic-ray identification with the low frequency aray
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2019-01-01
description 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.
url https://www.epj-conferences.org/articles/epjconf/pdf/2019/21/epjconf_arena2018_04005.pdf
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