The Superheterodyne Receiver
A 1918 architecture still in your phone. Don't tune the filter — move the signal to it, and pay for it with the image frequency.
Skip to the animationThe superheterodyne receiver mixes the incoming signal with a tuneable local oscillator so that the wanted station always lands on a fixed intermediate frequency — moving all the difficult filtering into one stage that never has to be retuned, at the cost of an image frequency.
The problem with tuning a filter
Selectivity is measured relative to the centre frequency. A 10 kHz channel at 1 MHz needs a Q of 100; the same channel at 100 MHz needs a Q of 10 000 — and a tuneable filter that stays that sharp across a band is not a practical component.
The trick
- 1Multiply the incoming signal by a local oscillator, producing sum and difference frequencies.
- 2Tune the oscillator so the wanted station's difference always lands at a fixed intermediate frequency.
- 3Filter and amplify at that fixed IF, with a filter that never has to move.
- 4Demodulate from the IF.
At a fixed frequency, a ceramic or crystal filter gives steep skirts and a flat passband cheaply. Most of the receiver's gain and all of its selectivity live in a stage designed once. AM broadcast standardised on 455 kHz, FM on 10.7 MHz.
The image frequency
Two input frequencies — one above the oscillator, one below — differ from it by the same amount, so both land on the IF. The unwanted one is the image, at 2 × IF from the wanted station, and nothing after the mixer can separate them.
- An RF preselector before the mixer rejects it. It can be broad, because the image is 2×IF away rather than one channel away.
- A higher IF pushes the image further out, making the preselector easier.
- But a higher IF makes the IF filter's job harder — the Q problem returns.
- Double conversion resolves it: a high first IF to kill the image, a low second IF for selectivity.
The supporting blocks
- RF preselector
- Broad tuned circuit before the mixer. Rejects the image; contributes little selectivity.
- Local oscillator
- The only tuned element that must track accurately, staying exactly one IF from the wanted station.
- Mixer
- A deliberately non-linear stage producing sum and difference products.
- IF amplifier and filter
- Fixed frequency, so it carries most of the gain and all of the selectivity.
- AGC
- A feedback loop measuring IF level and reducing gain ahead of it, so a 60 dB range of station strengths gives similar output.
- Detector
- Envelope for AM, discriminator or PLL for FM.
Why it survived
Armstrong's 1918 architecture is still in phones, Wi-Fi, radar and test equipment because the insight — translate the signal so the hard filter never moves — is independent of the technology implementing it.
What changed is that the IF is now often sampled directly and processed in software. Integrated receivers increasingly use zero-IF or low-IF architectures to avoid the image entirely, trading it for DC offset and I/Q imbalance problems instead.
The numbers you will be asked for
- Intermediate frequency
f_IF = |f_LO − f_RF|
- Image frequency
f_image = f_RF + 2·f_IF
for high-side injection
- Required Q
Q = f_centre / bandwidth
- Standard IFs
455 kHz (AM) · 10.7 MHz (FM)
Watch it work
Check yourself
question 1 / 4
One question at a time. Pick an answer to see why it is right or wrong, then move on — there is no score to keep and nothing is saved.