Wideband Radio Frequency Interference Detection for Microwave Radiometer Subsystem

Anthropogenic Radio-Frequency Interference (RFI) is threatening the quality and utility of multi-frequency passive microwave radiometry. The GPM Microwave Imager (GMI) on the Global Precipitation Measurement (GPM) mission launched on February 27, 2014 is already seeing RFI in the 10.7 and 18.7 GHz channels. It is important to understand that these frequency bands are strictly protected for science data measurement; yet, it is still corrupted by RFI. Indeed, this issue has led to the development of the first spaceborne digital RFI mitigation radiometer operating at 1.4 GHz for the Soil Moisture Active and Passive (SMAP) mission. We leverage our experience on SMAP to develop innovative technology for wider-bandwidth higher-frequency radiometers. The objective of this proposal is to develop a wideband (200-1000 MHz) digital detector subsystem and to demonstrate innovative RFI detection and removal techniques for microwave radiometers. The techniques proposed, complex valued kurtosis detector and independent component analysis (ICA), have the potential to improve the RFI detection rate in high frequency bandwidth. We are responding to a national imperative to develop RFI mitigation technology for future spaceflight radiometers. "Spectrum Management for the Twenty-first Century" recommends the continued development of so-called non-cooperative mitigation technologies. The Earth Science Technology roadmap for Advanced Microwave Components and Systems seeks "Demonstration of RFI mitigation approaches, and algorithms for future RFI environments to 40 GHz and beyond." These two National Research Council reports emphasize the importance of RFI mitigation technology for sustaining a reliable national passive microwave remote sensing capability.

Accelerate mission development and reduce risk by developing critical components and subsystems for advanced instruments and observing systems

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