Projecten per jaar
Samenvatting
Cosmic particles hitting Earth's moon produce radio emission via the Askaryan effect. If the resulting radio ns-pulse can be detected by radio telescopes, this technique potentially increases the available collective area for ZeV scale particles by several orders of magnitude compared to current experiments. The LOw Frequency ARray (LOFAR) is the largest radio telescope operating in the optimum frequency regime for this technique. In this contribution, we report on the status of the implementation of the lunar detection mode at LOFAR.
Originele taal-2 | English |
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Artikelnummer | 012077 |
Aantal pagina's | 6 |
Tijdschrift | Journal of Physics: Conference Series |
Volume | 1181 |
Nummer van het tijdschrift | 1 |
DOI's | |
Status | Published - 20 mrt 2019 |
Evenement | 26th Extended European Cosmic Ray Symposium - Altai State University, Barnaul, Russian Federation Duur: 6 jul 2018 → 10 jul 2018 https://ecrs18.asu.ru/event/1/ |
Bibliografische nota
Proceedings of the 26th Extended European Cosmic Ray Symposium (ECRS), Barnaul/Belokurikha, 2018Vingerafdruk
Duik in de onderzoeksthema's van 'Status of the Lunar Detection Mode for Cosmic Particles of LOFAR'. Samen vormen ze een unieke vingerafdruk.Projecten
- 1 Actief
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SRP8: SRP (Zwaartepunt): Hoge-Energiefysica
D'Hondt, J., Van Eijndhoven, N., Craps, B. & Buitink, S.
1/11/12 → 31/10/24
Project: Fundamenteel