The Superheterodyne Receiver — How Your Radio Hears
The Core Problem
Imagine trying to build a really sharp, narrow filter that can tune across the entire HF spectrum (3–30 MHz). That's incredibly difficult. Every time you change frequency, you'd need to re-tune the filter.
The superheterodyne ("superhet") receiver solves this elegantly: instead of moving the filter, it moves the signal to the filter.
How It Works — Step by Step
- RF Preselector — A broad filter that roughly selects the band you're listening to and rejects obvious out-of-band signals
- Mixer + Local Oscillator (LO) — The mixer combines the incoming signal with the LO. If you're tuned to 14.200 MHz and the IF is 9 MHz, the LO runs at 23.200 MHz. The difference: 23.200 − 14.200 = 9.000 MHz ✓
- IF Filter — This is fixed at 9 MHz and doesn't change when you tune. It provides the sharp selectivity. Crystal or DSP filters here determine your receive bandwidth (2.4 kHz for SSB, 500 Hz for CW, etc.)
- IF Amplifier — Boosts the filtered signal. AGC controls the gain here.
- Detector — Converts the IF signal back to audio. For SSB, this is a product detector (mixer with a BFO).
- Audio Amplifier — Drives the speaker or headphones.
The Image Problem
Here's the catch: the mixer doesn't know which signal produced the 9 MHz difference. If the LO is at 23.2 MHz, both a signal at 14.2 MHz AND a signal at 32.2 MHz produce a 9 MHz IF output!
The unwanted frequency is called the image, and it's always 2 × IF away from the desired signal.
The RF preselector must be good enough to reject the image. A higher IF makes this easier because the image is further away.
Dual Conversion — Best of Both Worlds
High-end receivers use two conversion stages:
- First IF: High (45-70 MHz) — puts the image far away, easy to reject
- Second IF: Low (9 MHz or 455 kHz) — allows narrow, affordable crystal filters
This gives both excellent image rejection AND excellent selectivity.