Page 100 - Photodetection and Measurement - Maximizing Performance in Optical Systems
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Source: Photodetection and Measurement

                                                                                      Chapter
                                                                                       5








              System Noise and Synchronous Detection












           5.1 Introduction

                       In Chap. 3 the fundamental noise contributions to our signal, shot noise of cur-
                       rents and thermal noise of resistors, were discussed. These noise sources in
                       general have no particular spectral character, delivering the same power per
                       unit bandwidth up to a very high frequency. However, the typical noise power
                       spectrum seen in a real photoreceiver in a real environment is far from being
                       as smooth as the quantum analysis leads us to expect. First, we have seen how
                       the frequency-dependent networks of electronic amplifiers and other compo-
                       nents connected to the photodiode can significantly modify the noise density as
                       a function of frequency. Further, the majority of semiconductor devices and even
                       many processes exhibit a 1/f character, which greatly increases noise density at
                       low frequencies, typically below about 500Hz. The voltage and current noise
                       spectral densities of both discrete transistors and opamps show this 1/f charac-
                       ter, with a corner frequency in this region.
                         Many man-made sources of electrical and optical interference are present at
                       the output of an optical receiver. At 50/60Hz, 100/120Hz, and 150/180Hz there
                       are often very strong electrical interference signals from line-voltage wiring and
                       power supply transformers. They can usually be greatly suppressed, if not
                       totally eliminated, by good electrostatic and/or ferromagnetic screening of
                       receivers, through diligent bypassing of power supply and signal leads entering
                       the receiver and through the avoidance of ground loops. In addition, many other
                       natural interfering light sources find their way to our detectors that vary in
                       intensity at a low frequency. These include sunlight (1/24 hour frequency), sun-
                       light modulated by clouds (ª1/minutes frequency) and flashing television and
                       computer screens (25 to 120Hz frame rate, 15 to 150kHz line rate).
                         All this suggests that measurements should be made, if possible, far away
                       from the low-frequency region 50 to 500Hz. Electrical interference can be fairly
                       quiet in the 3 to 50Hz region, but 1/f noise is large and the low frequencies
                       make measurements done there rather slow. Shifting the measurement of

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