In the UK, true in-band transmissions at 1418–1422 MHz are essentially nonexistent because this sits inside the internationally protected 1400–1427 MHz passive band allocated to radio astronomy and Earth-exploration (passive). That means:
- There are no licensed transmitters operating there.
- Any direct signal in that range would normally be illegal or due to equipment malfunction.
However — and this is the important practical point — intermodulation products can still appear there, even though nothing is meant to transmit in-band.
Where intermod can come from
Just above the passive band, the UK (via Ofcom) allocates:
- 1427–1452 MHz – mobile/fixed services (supplemental downlink, LTE/5G)
- 1452–1492 MHz – additional mobile allocations
Strong base stations in 1427–1452 MHz are the most common nearby high-power sources.
If two strong signals at frequencies f₁ and f₂ mix in a non-linear device (corroded joints, cheap masthead amps, overloaded SDR front ends, etc.), third-order products of the form:
2f_1 - f_2 \quad \text{or} \quad 2f_2 - f_1
can land inside 1418–1422 MHz.
This does not mean the transmitters are misbehaving — it usually means something in your receive chain (or occasionally metalwork nearby) is acting non-linearly.
How serious is it in practice?
For UK amateur hydrogen-line work:
🔹 Rural sites
- Generally low risk
- Intermod rarely limits observations
- External interference usually below the system temperature
🔹 Suburban sites
- Moderate risk
- Nearby L-band 4G/5G masts can be strong enough to:
- Drive LNAs into compression
- Generate third-order products
- Raise the baseline noise floor
🔹 Urban sites
- Can be a significant problem
- Particularly if:
- You have line-of-sight to a 1427+ MHz base station
- Your front end lacks sharp preselection
- You’re using wideband LNAs before filtering
Important distinction
Inside 1400–1427 MHz, there are:
- ❌ No legal active services
- ❌ No routine transmitters
- ✅ Very strict protection under ITU Region 1 allocations
So if you see structured signals between 1418–1422 MHz in the UK, they are usually:
- Front-end overload products
- Mixer images
- Poor-quality switch-mode PSU harmonics
- Reflections or re-radiation from nearby strong services above 1427 MHz
—not genuine in-band transmissions.
How bad numerically?
In a well-filtered system (e.g., hydrogen-line SAW preselection before the LNA):
- Intermod is typically below the galactic background level
- Not the dominant limitation
In an unfiltered wideband LNA directly at the antenna:
- You can easily raise the system temperature by 10–100 K equivalent
- Or see false spectral spikes that mimic narrow features
Practical mitigation (for 1420 MHz observing)
- Filter before the first active device
- Use a narrow hydrogen-line SAW filter (~50–70 MHz wide)
- Avoid high-gain wideband LNAs ahead of filtering
- Check for overload by reducing gain — if “signals” disappear, it’s intermod
Bottom line
In the UK, intermod in 1418–1422 MHz is usually a local equipment problem, not a spectrum-allocation problem.
The national protection of 1400–1427 MHz is strong — but modern L-band mobile transmitters just above 1427 MHz can create overload conditions if your front end isn’t well filtered.