First results from the FPGA/NIOS Adaptive FIR Filter Using Linear Prediction Implemented in the AERA Radio Stations to Reduce Narrow Band RFI for Radio Detection of Cosmic Rays
Zbigniew Szadkowski, D. G{\l}as, C. Timmermans, T. Wijnen (for the, Pierre Auger Collaboration)

TL;DR
This paper presents initial results of an adaptive linear prediction FIR filter implemented in FPGA/NIOS to suppress narrow-band RFI in radio detection of cosmic rays, improving signal clarity in the AERA experiment.
Contribution
It introduces a novel adaptive LP FIR filter deployed in real radio stations, demonstrating its effectiveness compared to traditional IIR notch filters for cosmic ray detection.
Findings
The adaptive LP FIR filter effectively reduces narrow-band RFI in real conditions.
The filter maintains stability over hours with constant coefficients.
Various filter configurations optimize power consumption and noise reduction.
Abstract
The FPGA/NIOS FIR filter based on linear prediction (LP) to suppress radio frequency interference (RFI) has been installed in several radio stations in the Auger Engineering Radio Array (AERA) experiment. AERA observes coherent radio emission from extensive air showers induced by ultra-high-energy cosmic rays to make a detailed study of the development of the electromagnetic part of air showers. Radio signals provide complementary information to that obtained from Auger surface detectors, which are predominantly sensitive to the particle content of an air shower at the surface. The radio signals from air showers are caused by the coherent emission due to geomagnetic and charge-excess processes. These emissions can be observed in the frequency band between 10 - 100 MHz. However, this frequency range is significantly contaminated by narrow-band RFI and other human-made distortions. A FIR…
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