Type a branch, a subject or a topic — “round robin”, “paging”, “civil”.

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 animation

The 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

  1. 1Multiply the incoming signal by a local oscillator, producing sum and difference frequencies.
  2. 2Tune the oscillator so the wanted station's difference always lands at a fixed intermediate frequency.
  3. 3Filter and amplify at that fixed IF, with a filter that never has to move.
  4. 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

loading visualisation…

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.

What is the superheterodyne's central idea?
What is the image frequency?
Raising the IF makes image rejection easier. What does it make harder?
Why does a strong station and a weak one come out of the same receiver at similar volume?

0 / 4

4 still unanswered — the dots above jump straight to them.