
A digital receiver in a 1.26-GHz spaceborne radar scatterometer now undergoing development includes a module for detecting radio-frequency interference (RFI) that could contam-inate scientific data intended to be acquired by the scatterometer. The role of the RFI-detection module is to identify time intervals during which the received signal is likely to be contaminated by RFI and thereby to enable exclusion, from further scientific data processing, of signal data acquired during those intervals. The underlying concepts of detection of RFI and rejection of RFI-contaminated signal data are also potentially applicable in advanced terrestrial radio receivers, including software-defined radio receivers in general, receivers in cellular telephones and other wireless consumer electronic devices, and receivers in automotive collision-avoidance radar systems.
The RFI-detection module is part of a digital square-law scatterometer processor (SP) implemented in a field-programmable gate array (FPGA). The raw scatterometer output signal used to generate an input signal for the SP is a down-converted signal at offset video frequencies in the range from 2 to 6 MHz. This signal is alternated in time with either radar echo pulses or a receiver “noise-only” measurement signal. The video signal is processed by an analog-to-digital converter (ADC) at a sampling rate of 16 MHz (greater than the Nyquist sampling rate) before being sent to the SP FPGA. The main part of the SP calculates the signal power by use of square-and-accumulate logic during each successive receiving time window. At the same time, raw magnitude (absolute-value) information from the ADC is fed to the RFI-detection module at the full 16-MHz sampling rate.