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Build the simplest CE amplifier with a 2N3904, voltage-divider bias, kΩ, V. Measure midband gain. Sweep input frequency from 10 Hz to 1 MHz, plot the magnitude response. You should see the low cutoff (set by coupling caps and emitter-bypass cap) and the high cutoff (set by Miller multiplication of ).
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Wrap negative feedback around it. Add a 1:10 feedback divider from output back to base via a coupling cap. Re-measure the gain, which should be much lower (closer to 10, set by 1/feedback ratio) but with much wider bandwidth. Verify that the gain-bandwidth product is approximately conserved.
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Build a Wien bridge oscillator with an op-amp and an incandescent flashlight bulb (the bulb's positive temperature coefficient stabilizes the amplitude, the lovely trick from Bill Hewlett's HP 200A). The output is a beautiful, low-distortion sine wave. Measure the frequency. Change the R or C and re-measure.
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Build a class-AB push-pull with a 2N3904 (NPN) and a 2N3906 (PNP). Drive it with a signal generator, observe the output on a scope. Notice how it crosses zero smoothly (no crossover distortion) when biased correctly with a couple of small-signal diodes between the bases, but distorts ugly if you remove the bias diodes.
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Try LTspice simulation of a simple cascode and a simple CE, both with the same transistor. Compare bandwidths. The cascode should be at least 5 to 10 times wider for the same low-frequency gain. Also compare their phase responses; the cascode keeps cleaner phase out to higher frequency.
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Build a single-tuned RF amplifier at 10 MHz with a slug-tuned inductor and an air-variable cap. Measure the bandwidth, then deliberately reduce the load resistance (lower the Q) and see the bandwidth widen. Verify .
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Measure the Miller effect directly. Build a CE amp without a cascode; sweep the source impedance (use a variable resistor in series with the input) from 100 Ω to 100 kΩ. Plot the high-frequency cutoff versus source impedance. The cutoff should fall as source impedance rises, by roughly , because the Miller-multiplied forms an RC with the source. This is the most direct experimental confirmation of Miller's theorem.
When the above feel intuitive, you are through this chapter.