Alternative Adaptive Filter Structures for Improved Radio Frequency Interference Cancellation in Radio Astronomy
D. A. Mitchell, J. G. Robertson, R. J. Sault

TL;DR
This paper explores five adaptive filter configurations for radio frequency interference cancellation in radio astronomy, demonstrating that dual-reference cancelers significantly improve RFI suppression below system noise levels.
Contribution
It introduces and compares five novel canceler setups, highlighting the advantages of dual-reference configurations for effective RFI mitigation.
Findings
RFI can be reduced below system noise by at least 20 dB.
Dual-reference cancelers outperform single-reference ones in RFI suppression.
Residual RFI in single-reference cancelers may limit sensitivity due to a nonzero noise floor.
Abstract
In radio astronomy, reference signals from auxiliary antennas that receive only the radio frequency interference (RFI) can be modified to model the RFI environment at the astronomy receivers. The RFI can then be canceled from the astronomy signal paths. However, astronomers typically only require signal statistics. If the RFI statistics are changing slowly, the cancellation can be applied to the signal correlations at a much lower rate than is required for standard adaptive filters. In this paper we describe five canceler setups; precorrelation and postcorrelation cancelers that use one or two reference signals in different ways. The theoretical residual RFI and added noise levels are examined and are demonstrated using microwave television RFI at the Australia Telescope Compact Array. The RFI is attenuated to below the system noise, a reduction of at least 20 dB. While dual-reference…
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