Noise in radar and intercept systems
Noise of all kinds limits ultimate detection performance for all electromagnetic sensor systems whether cosmic, UV, visible, IR, microwave or RF. Thermal noise is often thought of as the ultimate limitation on detection and tracking but often it is self-noise in a sensor system, which limits performance. Low-frequency systems with seemingly very low noise figures (NF) are often limited by sky noise from the residual of the “Big Bang,”from auroras and from what used to be called “Monkey Talk.”Great strides have been made in signal processing in the last 50 years. This is the result of dramatic improvements in signal processing hardware as well as a better theoretical understanding. In spite of this, many systems provide disappointing performance. The two main reasons for shortfalls are sensor signal processor self-noise and the physical world's continuing refusal to be normal (Gaussian). Although we have undreamed of device performance and number smashing today, we are inevitably forced by economics to limit hardware complexity that gives rise to significant self-noise. Noise and interference in the real world are “bursty,”“lumpy,”discrete, not stationary, anomalous and even malevolent! This chapter is an introduction to analog and digital signal processing self-noise analysis and heuristic means to control ill-behaved internal and external noise.
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