Understanding Noise Figure (NF): When It Matters and When It Doesn’t

What is Noise Figure (NF)?

Noise Figure (NF) quantifies how much noise an amplifier adds to the signal it processes. It is defined as:

NF (dB) = 10 * log10(SNR_in / SNR_out)

An NF of 3 dB means the amplifier degrades the signal-to-noise ratio (SNR) by a factor of 2.

NF is Frequency Dependent

Most datasheets only mention one NF value, but this hides a critical fact:

NF varies with frequency. It's typically low at low frequencies, rises toward the upper HF and VHF range, and often worsens above 500 MHz.

Especially in MMICs and opamps, capacitive coupling, parasitics, and gain roll-off all increase NF at higher frequencies.

Where NF Matters and Where It Doesn't

Frequency Dominant Noise Source Is NF Important?
< 10 MHz Atmosphere (QRN), man-made noise ❌ Mostly irrelevant
10–30 MHz Mix of atmospheric and system noise ⚠️ Depends on CMR & site
30–150 MHz Receiver NF, galactic & man-made noise ✅ Important for weak signals
>150 MHz Receiver + antenna + losses ✅ Critical in EME, VHF DX

Below 30 MHz: It's Not the LNA, It's the World

At LF, MF, and most of HF:

  • Atmospheric noise floor is around -100 to -120 dBm/Hz.
  • Even a "bad" NF of 10 dB has no real impact on total SNR if your antenna picks up more noise than the LNA adds.
  • Improving NF beyond ~6 dB often yields no reception benefit.

What is critical at these frequencies:

  • Common-mode rejection ratio (CMRR) to suppress RFI picked up on the feedline
  • Proper antenna design to pick up magnetic (H-field) or electric (E-field) energy with good SNR

Above 30 MHz: NF Starts to Matter

As you enter VHF and UHF:

  • Atmospheric noise vanishes
  • The galactic background becomes dominant until about 300 MHz
  • Above that, your receiver’s NF sets the limit — especially in quiet rural sites or for EME, SAT, or weak signal DX

Myth: "Lower NF always means better reception"

Nope. That’s marketing nonsense.

Unless your system noise floor (antenna + sky + RFI + losses) is below your LNA noise floor, improving NF gives you nothing.

What does matter:

  • Low NF in VHF/UHF/Microwave
  • High CMRR and shielding in HF and below
  • Proper impedance match to prevent reflections and losses

Practical Example: HF SDR Preamp

Scenario Antenna Type NF (dB) Result
Quiet site, active whip EchoTracer 1.7 dB Excellent SNR — atmospheric-limited
Urban, no CMR choke Same whip 0.5 dB Poor SNR — common-mode noise dominates
VHF DX Yagi, no LNA 4-el beam @ 144 MHz Weak signals lost in receiver noise
VHF Yagi + 0.8 dB NF LNA Same beam 0.8 dB Weak DX now decodable

Conclusion: Focus on What Actually Affects SNR

NF is just one piece of the puzzle.

NF is key:

  • For VHF/UHF/SHF
  • In low-noise, quiet environments
  • With weak signal modes like EME, FT8 DX, satellites

NF is overrated:

  • For HF reception, especially below 10 MHz
  • In urban QRM zones
  • When CMR is poor

A 1 dB NF won't save you if your antenna hears more streetlights than sky.

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Written by Joeri Van DoorenON6URE – RF, electronics and software engineer, complex platform and antenna designer. Founder of RF.Guru. An expert in active and passive antennas, high-power RF transformers, and custom RF solutions, he has also engineered telecom and broadcast hardware, including set-top boxes, transcoders, and E1/T1 switchboards. His expertise spans high-power RF, embedded systems, digital signal processing, and complex software platforms, driving innovation in both amateur and professional communications industries.