Detecting radio emission from air showers with LOFARShow others and affiliations
2013 (English)In: 5th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities: ARENA 2012 / [ed] Robert Lahmann, Thomas Eberl, Kay Graf, Clancy James, Tim Huege, Timo Karg, Rolf Nahnhauer, American Institute of Physics (AIP), 2013, Vol. 1535, p. 105-110Conference paper, Published paper (Refereed)
Resource type
Text
Abstract [en]
LOFAR (the Low Frequency Array) is the largest radio telescope in the world for observing low frequency radio emission from 10 to 240 MHz. In addition to its use as an interferometric array, LOFAR is now routinely used to detect cosmic ray induced air showers by their radio emission. The LOFAR core in the Netherlands has a higher density of antennas than any dedicated cosmic ray experiment in radio. On an area of 12 km2 more than 2300 antennas are installed. They measure the radio emission from air showers with unprecedented precision and, therefore, give the perfect opportunity to disentangle the physical processes which cause the radio emission in air showers. In parallel to ongoing astronomical observations LOFAR is triggered by an array of particle detectors to record time-series containing cosmic-ray pulses. Cosmic rays have been measured with LOFAR since June 2011. We present the results of the first year of data.
Place, publisher, year, edition, pages
American Institute of Physics (AIP), 2013. Vol. 1535, p. 105-110
Series
AIP Conference Proceedings, ISSN 0094-243X ; 1535
National Category
Astronomy, Astrophysics and Cosmology
Research subject
Physics, Astroparticle Physics
Identifiers
URN: urn:nbn:se:lnu:diva-51559DOI: 10.1063/1.4807530OAI: oai:DiVA.org:lnu-51559DiVA, id: diva2:915317
Conference
5th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities: ARENA 2012
2016-03-292016-03-292019-02-27Bibliographically approved