Corstanje A, Van Den Akker M, B̈ahren L, Falcke H, Frieswijk W, Ḧorandel JR, Horneffer A, James CW, Kelley JL, Mcfadden R, Mevius M, Nelles A, Schellart P, Scholten O, Thoudam S, Ter Veen S (2011)
Publication Type: Conference contribution
Publication year: 2011
Publisher: Institute of High Energy Physics
Book Volume: 3
Pages Range: 192-195
Conference Proceedings Title: Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011
Event location: CHN
DOI: 10.7529/ICRC2011/V03/0916
LOFAR (the Low Frequency Array), a distributed digital radio telescope with stations in the Netherlands, Germany, France, Sweden, and the United Kingdom, is designed to enable full-sky monitoring of transient radio sources. These capabilities are ideal for the detection of broadband radio pulses generated in cosmic ray air showers. The core of LOFAR consists of 24 stations within 4 square kilometers, and each station contains 96 low-band antennas and 48 high-band antennas. This dense instrumentation will allow detailed studies of the lateral distribution of the radio signal in a frequency range of 10-250 MHz. Such studies are key to understanding the various radio emission mechanisms within the air shower, as well as for determining the potential of the radio technique for primary particle identification. We present the status of the LOFAR cosmic ray program, including the station design and hardware, the triggering and filtering schemes, and our initial observations of cosmic-ray-induced radio pulses.
APA:
Corstanje, A., Van Den Akker, M., B̈ahren, L., Falcke, H., Frieswijk, W., Ḧorandel, J.R.,... Ter Veen, S. (2011). LOFAR: Detecting cosmic rays with a radio telescope. In Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011 (pp. 192-195). CHN: Institute of High Energy Physics.
MLA:
Corstanje, A., et al. "LOFAR: Detecting cosmic rays with a radio telescope." Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011, CHN Institute of High Energy Physics, 2011. 192-195.
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