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 coreof LOFAR consists of 24 stations within 4 square kilometers, and each station contains 96 low-band antennas and 48high-band antennas. This dense instrumentation will allow detailed studies of the lateral distribution of the radio signalin a frequency range of 10-250 MHz. Such studies are key to understanding the various radio emission mechanismswithin 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 andfiltering schemes, and our initial observations of cosmic-ray-induced radio pulses.
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