Wide-Area GNSS Interference Monitoring with CYGNSS GNSS-R Delay-Doppler Noise Floor Observations
Ji-Hyeon Shin, Pyo-Woong Son

TL;DR
This paper introduces a maximum-based aggregation method for CYGNSS DDM noise-floor data to improve spaceborne GNSS RFI detection, demonstrating enhanced detection performance over existing mean and kurtosis-based methods.
Contribution
It replaces mean aggregation with maximum aggregation of DDM noise-floor values, preserving anomalies and improving RFI detection accuracy.
Findings
Maximum aggregation detects more RFI events than mean aggregation.
The method achieves higher detection rates in documented interference environments.
It offers a simple, lightweight improvement over existing CYGNSS RFI detection techniques.
Abstract
Delay-Doppler Map (DDM) noise-floor observations from the Cyclone Global Navigation Satellite System (CYGNSS) constellation provide a practical means for spaceborne detection of GNSS radio frequency interference (RFI). Existing CYGNSS analyses use NASA's kurtosis-based flag product or mean aggregation of the four simultaneous DDM noise-floor values at each epoch. However, these DDMs are formed from different reflected GNSS signals received through two nadir antennas with different orientations. Thus, ground-based RFI may raise only some channel noise floors, depending on antenna gain and viewing geometry. Mean aggregation can dilute the strongest anomaly with unaffected channels, causing missed detections. This paper replaces the mean with the maximum of four co-temporal DDM noise-floor values. This statistic preserves channel-level anomalies and accounts for channel-dependent exposure.…
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