First Results from the FPGA/NIOS Adaptive FIR Filter Using Linear Prediction Implemented in the Auger Engineering Radio Array

In this paper we present first results of the efficiency of the adaptive FIR filter based on the linear prediction (LP) for a suppression of radio frequency interference (RFI), deployed in real AERA (Auger Engineering Radio Array) station on pampas, with a comparison to the currently used IIR notch filter with constant coefficients. The filter has been installed in several radio stations in the 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 filter implemented in the FPGA logic segment of the front-end electronics of a radio sensor significantly improves the signal-to-noise ratio. Theoretical calculations show a high efficiency of this filter for mono-carrier as well as for standard FM radio contaminations. The laboratory tests, performed on an Altera development kit confirmed the theoretical expectations. The coefficients for the linear predictor are dynamically refreshed and calculated in a Voipac PXA270M ARM processor, which is implemented on a daughter-board placed in the same digital unit as the FPGA. Laboratory tests confirms the stability of the filter. Using constant LP coefficients the suppression efficiency remains the same for hours, which corresponds to more than 1012 clock cycles. We compare in real conditions several variants of the LP FIR filter with various lengths and various coefficients widths (due to fixed-point representations in the FPGA logic) with the aim to minimise the power consumption for the radio station while keeping sufficient accuracy for noise reduction.

[1]  J. Makhoul,et al.  Linear prediction: A tutorial review , 1975, Proceedings of the IEEE.

[2]  P. Abreu,et al.  The exposure of the hybrid detector of the Pierre Auger Observatory , 2010, 1010.6162.

[3]  S. Fliescher,et al.  Radio detection of cosmic ray induced air showers at the Pierre Auger Observatory , 2012 .

[4]  G. Askar’yan.  Coherent Radio Emission from Cosmic Showers in Air and in Dense Media , 1965 .

[5]  O. Ravel,et al.  Radioelectric field features of extensive air showers observed with CODALEMA , 2006, astro-ph/0608550.

[6]  H. Gemmeke,et al.  FPGA Based Signal-Processing for Radio Detection of Cosmic Rays , 2011, IEEE Transactions on Nuclear Science.

[7]  Z. Szadkowski,et al.  FPGA/NIOS implementation of an adaptive FIR filter using linear prediction to reduce narrow band RFI for radio detection of cosmic rays , 2012, 2012 18th IEEE-NPSS Real Time Conference.

[8]  N. T. Thao,et al.  Probing the radio emission from air showers with polarization measurements , 2014 .

[9]  Marko Zavrtanik,et al.  Properties and performance of the prototype instrument for the Pierre Auger Observatory , 2004, Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment.

[10]  Keshab K. Parhi,et al.  Pipeline interleaving and parallelism in recursive digital filters. I. Pipelining using scattered look-ahead and decomposition , 1989, IEEE Trans. Acoust. Speech Signal Process..

[11]  I. Lerche,et al.  Radiation from cosmic ray air showers , 1966, Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences.

[12]  Van Den,et al.  Analysis of the efficiency of the filters suppressing the RFI being developed for the extension of AERA , 2013 .

[13]  S. Buitink,et al.  Detection and imaging of atmospheric radio flashes from cosmic ray air showers , 2005, Nature.

[14]  J. Bougeret,et al.  Calibration of low-frequency radio telescopes using the galactic background radiation , 2001 .

[15]  D. Fegan.  Detection of elusive radio and optical emission from cosmic-ray showers in the 1960s , 2011, 1104.2403.

[16]  D. Glas,et al.  An optimization of the FPGA/NIOS adaptive FIR filter using linear prediction to reduce narrow band RFI for the next generation ground-based ultra-high energy cosmic-ray experiment , 2013 .