Cosmic ray physics with the LOFAR radio telescope

T. Winchen, A. Bonardi, S. Buitink, A. Corstanje, H. Falcke, B. M. Hare, J. R. Hörandel, P. Mitra, K. Mulrey, A. Nelles, J. P. Rachen, L. Rossetto, P. Schellart, O. Scholten, S. Ter Veen, S. Thoudam, T. N.G. Trinh

Research output: Contribution to journalConference articlepeer-review

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Abstract

The LOFAR radio telescope is able to measure the radio emission from cosmic ray induced air showers with hundreds of individual antennas. This allows for precision testing of the emission mechanisms for the radio signal as well as determination of the depth of shower maximum X max, the shower observable most sensitive to the mass of the primary cosmic ray, to better than 20 g cm-2. With a densely instrumented circular area of roughly 320 m2, LOFAR is targeting for cosmic ray astrophysics in the energy range 1016-1018 eV. In this contribution we give an overview of the status, recent results, and future plans of cosmic ray detection with the LOFAR radio telescope.

Original languageBritish English
Article number012020
JournalJournal of Physics: Conference Series
Volume1181
Issue number1
DOIs
StatePublished - 10 Mar 2019
Event26th Extended European Cosmic Ray Symposium, E+CRS 2018 - Barnaul-Belokurikha, Russian Federation
Duration: 6 Jul 201810 Jul 2018

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