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EL4452CS Datasheet(PDF) 9 Page - Intersil Corporation |
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EL4452CS Datasheet(HTML) 9 Page - Intersil Corporation |
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9 / 10 page ![]() 9 AGC Circuits The basic AGC (automatic gain control) loop is this: A multiplier scales the input signal and provides necessary gain and buffers the signal presented to the output load, a level detector (shown schematically here as a diode) converts some measure of the output signal amplitude to a DC level, a low-pass filter attenuates any signal ripple present on that DC level, and an amplifier compares that level to a reference and amplifies the error to create a gain- control voltage for the multiplier. The circuitry is a servo that attempts to keep the output amplitude constant by continuously adjusting the multiplier’s gain control input. Most AGC’s deal with repetitive input signals that are capacitively coupled. It is generally desirable to keep DC offsets from mixing with AC signals and fooling the level detector into maintaining the DC output offset level constant, rather than a smaller AC component. To that end, either the level detector is AC-coupled, or the reference voltage must be made greater than the maximum multiplier gain times the input offset. For instance, if the level detector output equaled the reference voltage at 1V of EL4452 output, the 8mV of input offset would require a maximum gain of 125 through the EL4452. Bias current-induced offsets could increase this further. Depending on the nature of the signal, different level detector strategies will be employed. If the system goal is to prevent overload of subsequent stages, peak detectors are preferred. Other strategies use an RMS detector to maintain constant output power. Here is a simple AGC using peak detection (Figure 2). The output of the EL4452 drives a diode detector which is compared to VREF by an offset integrator. Its output feeds the gain-control input of the EL4452. The integrator’s output is attenuated by the 2k Ω and 2.7kΩ resistors to prevent the op-amp from overloading the gain-control pin during zero input conditions. The 510k Ω resistor provides a pull-down current to the peak level storage capacitor C1 to allow it to drift negative when output amplitude reduces. Thus the detector is of fast attack and slow decay design, able to reduce AGC gain rapidly when signal amplitude suddenly increases, and increases gain slowly when the input drops out momentarily. The value of C1 determines drop-out reaction rates, and the value of CF affects overall loop time constant as well as the amount of ripple on the gain-control line. C2 can be used to reduce this ripple further, although it contributes to loop overshoot when input amplitude changes suddenly. The op-amp can be any inexpensive low- frequency type. The major problem with diode detectors is their large and variable forward voltage. They require at least a 2VP-P peak output signal to function reliably, and the forward voltage should be compensated by including a negative VD added to VREF. Even this is only moderately successful. At the expense of bandwidth, op-amp circuits can greatly improve diode rectifiers (see “An Improved Peak Detector”, an FIGURE 1. BASIC AGC LOOP FIGURE 2. EL4452 |
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