DocumentCode :
2153299
Title :
Radio frequency interference (RFI) in digital microwave radiometers
Author :
Piepmeier, J.R.
Author_Institution :
Microwave Instrum. Technol. Branch, NASA Goddard Space Flight Center, Greenbelt, MD, USA
Volume :
3
fYear :
2004
fDate :
20-24 Sept. 2004
Firstpage :
1691
Abstract :
Here, we developed a model for determining the effects of a narrow-band RFI on low resolution digital correlators. Low resolution correlators rely on a theoretical inversion to obtain the input correlation coefficient from the digital output. This inversion is based on the Gaussian statistics of the input signals. In the presence of the narrow-band interference, the statistics are not Gaussian and the theoretical inversion is no longer valid. The result is an error in the correlator output. We studied this phenomenon for four correlator resolutions: 1, 1.5, 2, and 4 bits. The errors are significant for 1, 1.5, and 2-bit systems. We found in the presence of relatively strong interference (INR≳0 dB) the errors can be ten´s of percent. The error reduces to less than 0.03% for INR<-16 dB. For the four-bit correlators, the errors are less than 0.03% for all cases studied. The error is also nonlinearly dependent upon input correlation coefficient.
Keywords :
correlators; error statistics; geophysical equipment; radiofrequency interference; radiometers; remote sensing; Gaussian statistics; digital microwave radiometer; digital output; four-bit correlators; input correlation coefficient; low resolution digital correlators; narrow-band RFI; narrow-band interference; radio frequency interference; Correlators; Narrowband; Radiofrequency interference; Radiometers; Random processes; Signal processing; Signal resolution; Space technology; Spectroscopy; Statistics;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Geoscience and Remote Sensing Symposium, 2004. IGARSS '04. Proceedings. 2004 IEEE International
Print_ISBN :
0-7803-8742-2
Type :
conf
DOI :
10.1109/IGARSS.2004.1370656
Filename :
1370656
Link To Document :
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