LOFAR: Detecting Cosmic Rays with a Radio Telescope
Abstract
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.
Keywords
Cite
@article{arxiv.1109.5805,
title = {LOFAR: Detecting Cosmic Rays with a Radio Telescope},
author = {A. Corstanje and M. van den Akker and L. Bähren and H. Falcke and W. Frieswijk and J. R. Hörandel and A. Horneffer and C. W. James and J. L. Kelley and R. McFadden and M. Mevius and A. Nelles and P. Schellart and O. Scholten and S. Thoudam and S. ter Veen},
journal= {arXiv preprint arXiv:1109.5805},
year = {2011}
}
Comments
Contribution to the 32nd International Cosmic Ray Conference (Beijing, China, 11-18 Aug. 2011); 4 pages, 4 figures