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Towards real-time cosmic-ray identification with the LOw Frequency ARay
Radboud Univ Nijmegen, Netherlands.
Vrije Univ Brussel, Belgium.
Radboud Univ Nijmegen, Netherlands.
Radboud Univ Nijmegen, Netherlands;NIKHEF, Netherlands;Netherlands Inst Radio Astron ASTRON, Netherlands.
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2019 (English)In: 8th International Conference on Acoustic and Radio EeV Neutrino Detection Activities (ARENA 2018) / [ed] Riccobene, G Biagi, S Capone, A Distefano, C Piattelli, P, EDP Sciences , 2019, p. 1-3, article id 04005Conference paper, Published paper (Refereed)
Abstract [en]

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.

Place, publisher, year, edition, pages
EDP Sciences , 2019. p. 1-3, article id 04005
Series
EPJ Web of Conferences, E-ISSN 2100-014X ; 216
National Category
Astronomy, Astrophysics and Cosmology
Research subject
Physics, Astroparticle Physics
Identifiers
URN: urn:nbn:se:lnu:diva-98766DOI: 10.1051/epjconf/201921604005ISI: 000570244200041Scopus ID: 2-s2.0-85184350781ISBN: 978-2-7598-9080-4 (print)OAI: oai:DiVA.org:lnu-98766DiVA, id: diva2:1498838
Conference
8th International Conference on Acoustic and Radio EeV Neutrino Detection Activities (ARENA), JUN 12-18, 2015, Ist Nazl Fisica Nucl, Lab Nazl Sud, Catania, ITALY
Available from: 2020-11-05 Created: 2020-11-05 Last updated: 2024-02-15Bibliographically approved

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Thoudam, Satyendra

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CiteExportLink to record
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