An air shower array for LOFAR: LORA
S. Thoudam, Guus van Aar, M. van den Akker, L. Bähren, A. Corstanje, Heino D. Falcke, J.R. Hörandel, A. Horneffer, Clancy W. James, M. Mevius, Olaf Scholten, K. Singh, Sander Ter Veen
Abstract
S. Thoudam, Guus van Aar, M. van den Akker, L. Bähren, A. Corstanje, Heino D. Falcke, J.R. Hörandel, A. Horneffer, Clancy W. James, M. Mevius, Olaf Scholten, K. Singh, Sander Ter Veen
Abstract
LOFAR is a new form of radio telescope which can detect radio emission from air showers induced by very high-energy cosmic rays. It can also look for radio emission from particle cascades on the Moon induced by ultra high-energy cosmic rays or neutrinos. To complement the radio detection, we are setting up a small particle detector array LORA (LOfar Radboud Air shower array) within an area of $\sim 300$ m diameter in the LOFAR core. It will help in triggering and confirming the radio detection of air showers with the LOFAR antennas. In this paper, we present a short overview about LORA and discuss its current status.
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LOFAR is a new form of radio telescope which can detect radio emission from air showers induced by very high-energy cosmic rays. It can also look for radio emission from particle cascades on the Moon induced by ultra high-energy cosmic rays or neutrinos. To complement the radio detection, we are setting up a small particle detector array LORA (LOfar Radboud Air shower array) within an area of $\sim 300$ m diameter in the LOFAR core. It will help in triggering and confirming the radio detection of air showers with the LOFAR antennas. In this paper, we present a short overview about LORA and discuss its current status.
Key concepts: LOFAR, Air shower, Physics, Cosmic ray, Radio telescope, Astroparticle physics, Astrophysics, Detector