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Interlude: Alternative Circuits and Detection Techniques

                                               Interlude: Alternative Circuits and Detection Techniques  85

                       integrate both an LED and a photodetector into the same package. The LED
                       was used as the primary sensor for track servoing to read out reflective tracks
                       printed onto flexible disk media.
                         If you try this by just biasing the LED and looking at the LED voltage AC
                       coupled to an oscilloscope input you are unlikely to see any signal. With proper
                       receiver design, however, signals can be detected. The rules are exactly the same
                       as those used in Chap. 3, although the requirements and design solutions
                       are rather different from the high-resistance, high-sensitivity designs of the
                       discussion up to now.
                         The forward-biased LED photodetector passes a static current of several mil-
                       liamps, and we have to contend with the resulting full shot noise. The pho-
                       tocurrent generator acts in parallel with the forward-biased perfect diode of
                       our photodiode model. Hence it acts as a generator with very low impedance,
                       approximately the few ohm dynamic impedance of the diode (25/I(mA)W),
                       and a receiver must be optimized to work with this low source impedance.
                       Similar requirements exist for low-noise detection of signals from moving-
                       coil record player heads, moving-ribbon microphones, and certain types of
                       photoconductors.
                         The dominant parameter determining noise performance here is the voltage
                       noise density of the input amplifier stage. Most operational amplifiers have
                       voltage noise spectral densities in the range 10 to 50nV/ Hz , but better per-
                       formance can be obtained with discrete transistors. As we saw in Chap. 3 the
                       input-equivalent noise sources of junction transistors are the shot noise of the
                       base current and the thermal noise of the effective base resistance. These are
                       given by:
                                                          2  qI e
                                                i n =  2 qI b =                            (4.1)
                                                2
                                                           b
                                                                    kT
                                               e n =  4  kT Ê Ë  r b +  r e ˆ ¯  : r e =  qI e  (4.2)
                                                2
                                                           2
                       I b and I e are the transistor base and emitter currents, and r b , r e are the base
                       spreading resistance and emitter small-signal resistance.  b is the transistor
                       current gain. Figure 4.6 shows the variation of i n and e n with transistor emitter
                       current.
                         For the ª1W source resistance of the forward-biased LED, the current shot
                       noise is negligible and thermal noise is dominant. The design clearly needs the
                       input transistor to be run at high current. When this is optimized, signal-to-
                       noise is limited by its base-spreading resistance r bb. This can be minimized by
                       connecting several transistors in parallel and/or by choosing devices specially
                       processed for low r bb. Large die power transistors are sometimes used for this
                       purpose, but specialist devices are better. Devices such as the 2SD786 and
                       2SB737 transistors are available with r bb of 4W and 2W respectively, which leads
                       to e n <  1nV/ Hz . Figure 4.5 shows a high-gain common emitter amplifier
                       designed around the LM394 bipolar supermatch pair. A balanced configuration
                       using a second LED reduces the effects of temperature drifts, but the circuit is

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