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Cosmic ray physics with the LOFAR radio telescope
Vrije Universiteit Brussel, Belgium.
Radboud University, The Netherlands.
Vrije Universiteit Brussel, Belgium.
Radboud University, The Netherlands.
Vise andre og tillknytning
2019 (engelsk)Inngår i: 26th Extended European Cosmic Ray Symposium, 6–10 July 2018, Altai State University, Barnaul-Belokurikha, Russian Federation, Institute of Physics (IOP), 2019, nr 1Konferansepaper, Publicerat paper (Fagfellevurdert)
Abstract [en]

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 m 2 , LOFAR is targeting for cosmic ray astrophysics in the energy range 10 16 -10 18 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. © Published under licence by IOP Publishing Ltd.

sted, utgiver, år, opplag, sider
Institute of Physics (IOP), 2019. nr 1
Serie
Journal of Physics: Conference Series, ISSN 1742-6588, E-ISSN 1742-6596 ; 1181
Emneord [en]
Cosmic ray detectors, Cosmology, Radio telescopes, Air showers, Emission mechanism, Energy ranges, Radio emission, Radio signals, Cosmic rays
HSV kategori
Forskningsprogram
Fysik, Astropartikelfysik
Identifikatorer
URN: urn:nbn:se:lnu:diva-86424DOI: 10.1088/1742-6596/1181/1/012020Scopus ID: 2-s2.0-85064343283OAI: oai:DiVA.org:lnu-86424DiVA, id: diva2:1337035
Konferanse
26th Extended European Cosmic Ray Symposium, E+CRS 2018, 6-10 July 2018
Merknad

Conference code: 146680; Export Date: 22 May 2019; Conference Paper

Tilgjengelig fra: 2019-07-11 Laget: 2019-07-11 Sist oppdatert: 2019-09-02bibliografisk kontrollert

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