A ratio
Compares one power or voltage level with another. It has no absolute reference by itself.
RF Engineering Guide
A practical introduction to the dB scale and how it applies to inter-station interference, transmitter products, receiver blocking, intermodulation and safe receiver input levels.


Basics and terminology
Whenever two or more transceivers are used in close proximity, some level of coupling and interference is involved. In a well-designed station this may be barely noticeable. In a poor layout it can cause receiver overload, desensing, intermodulation, or even physical damage to receiver input components.
The problem is not only the wanted transmitted signal. Real transmitters also produce harmonics, phase noise and wideband noise. Real receivers also have limits: they can block, mix unwanted signals, become desensitised, or be damaged if excessive RF reaches the antenna input.
In simple terms, dB, dBm, dBm/Hz and dBc provide a common language for measuring very large differences in signal level. This is essential when planning filters, antenna spacing, coax separation and receiver protection.
Understanding the dB scale
Radio stations deal with enormous differences in power. A transmitter may produce hundreds or thousands of watts while a receiver is trying to hear signals close to its internal noise floor. These values are awkward to compare directly in watts or volts, so RF engineers normally use logarithmic units.
Compares one power or voltage level with another. It has no absolute reference by itself.
Power referenced to 1 milliwatt. Therefore, 1 mW equals 0 dBm.
Describes the amount of noise power present in a 1 Hz bandwidth.
Harmonics, sidebands and noise around a carrier are often specified relative to carrier power.
Power ratio in dB = 10 log??(P? ÷ P?)Voltage ratio in dB = 20 log??(V? ÷ V?) when both voltage measurements use the same impedance.
10 log??(1500 ÷ 0.001)10 log??(100 ÷ 0.001)10 log??(3 × 10?¹? ÷ 0.001)The 1,500 W example comes from the original American reference and is retained as a mathematical example. Always operate within the power limits and conditions of your own amateur-radio licence.
Convert absolute power between dBm, watts and milliwatts in a 50 Ω RF system.
dBm = 10 log₁₀(P watts ÷ 0.001)
Noise and bandwidth
For a narrow-band signal such as CW, power can be calculated directly from the power read on a wattmeter. Wideband noise is different. The amount of noise admitted by a receiver depends on both noise density and receiver bandwidth.
If a receiver measures ?50 dBm of noise in a 500 Hz bandwidth:
Noise density = ?50 dBm ? 10 log??(500) Noise density = ?50 dBm ? 26.99 dB Noise density ? ?77 dBm/HzThe wider the receiver bandwidth, the more total noise power is admitted. Filter bandwidth therefore matters when assessing interference, sensitivity and receiver performance.
Calculate noise density from measured noise, or total noise from a known density.
Transmitter products
Even a good transmitter produces unwanted products alongside the wanted signal. These products can interfere with nearby receivers, especially in contest stations, multi-radio club stations and special-event stations with several transmitters active at the same time.
Harmonics occur at integer multiples of the transmitted frequency. A 7 MHz transmitter can produce harmonic energy near 14 MHz and 21 MHz, potentially affecting receivers on those bands.
The original reference gives a worst-case example of harmonics at ?40 dBc. From a 1,500 W carrier this corresponds to approximately 150 mW, or +21.8 dBm.
Oscillators and frequency synthesisers are not perfectly clean. Small random phase variations create noise sidebands around the transmitted carrier.
Phase noise is generally strongest close to the carrier and reduces with increasing frequency offset. This is a major issue when two stations operate close together on the same band.
Solid-state transmitters use wideband gain stages. Noise generated in early stages can be amplified through the transmit chain and appear at the final output.
Low-pass filtering reduces harmonics and some out-of-band energy, but band-pass filtering and physical isolation remain important in a serious multi-radio station.
Receiver limits
A receiver is designed to handle weak signals. A large unwanted signal at its antenna input can produce several different failure modes, ranging from increased noise and cross-products through to complete blocking or damage to input components.
The levels below are examples quoted from the source material. Actual limits depend on receiver design, preamplifier state, attenuator settings, frequency separation, protection components and manufacturer specifications. Consult the service manual or manufacturer data for the equipment being protected.
| Problem | Example level from source text | What happens |
|---|---|---|
| Receiver damage | Approximately +17 dBm maximum-safe-input example | Input resistors, switching diodes, protection devices or front-end components may be overstressed. |
| Receiver blocking | Approximately +5 dBm at 50 kHz offset and 0 dBm at 20 kHz offset | The receiver front end or signal path is overloaded and normal reception becomes unusable. |
| Intermodulation distortion | Approximately ?35 dBm | Two or more strong signals mix in a non-linear device and create false signals such as 2F? ? F? and 2F? ? F?. |
| Noise floor | Approximately ?135 dBm | The receiver's internal noise and selected bandwidth set the lower limit of what can be heard. |
With one strong signal at 7020 kHz and another at 7030 kHz, third-order products may appear at:
2F? ? F? = 7010 kHz2F? ? F? = 7040 kHzThey often fall close to the original signals and can land inside the same amateur band, where ordinary low-pass filtering cannot remove them after they have been generated in the receiver.
Enter two strong signal frequencies. The calculator shows the common 2F₁ − F₂ and 2F₂ − F₁ products.
Power-level chart
The dBm scale makes it possible to compare transmitter output, harmonic energy, receiver-blocking levels, intermodulation thresholds and receiver noise floors on one common scale.
To reduce a +61.76 dBm transmitter signal to the source text's +17 dBm receiver-input example:
61.76 dBm ? 17 dBm = 44.76 dB Approximately 45 dB isolation requiredAvoiding physical damage is not enough. Clean simultaneous operation normally requires much greater isolation to control blocking, intermodulation, transmitter phase noise and degradation of the receiver noise floor.
Compare the isolation required from transmitter output to a chosen receiver-input target with the isolation available in the station.
Summary
They produce harmonics, phase noise and wideband noise as well as the wanted carrier.
Strong unwanted signals can cause blocking, intermodulation, desensing or damage.
Using dB and dBm allows the required isolation between transmitters and receivers to be calculated.
Good band-pass filtering, coax separation, antenna spacing, bonding and station layout all reduce interference risk.
Reference and credit
This educational page is based on a free excerpt of Managing Interstation Interference by George Cutsogeorge, W2VJN.
Original reference: International Radio — INRAD.