Noise figure (NF)
The factor by which an optical amplifier degrades the input signal-to-noise ratio, in dB. The figure of merit for amplifier quality.
Noise figure in decibels is
where is the linear noise factor and SNR is the signal-to-noise ratio at the photodetected output.
For an optical amplifier with gain and spontaneous emission factor :
In the high-gain limit ():
with a fundamental quantum-mechanical lower bound of (full population inversion), giving NF dB. Real amplifiers exceed this due to partial inversion and additional loss mechanisms.
Typical values:
| Amplifier | NF |
|---|---|
| EDFA (low-noise pre-amp) | 3.5 – 5 dB |
| EDFA (general telecom) | 4 – 6 dB |
| EDFA (booster, high gain) | 5 – 7 dB |
| Semiconductor optical amplifier (SOA) | 7 – 12 dB |
| Distributed Raman amplifier | to dB (effective) |
| YDFA (ytterbium-doped) | 4 – 8 dB |
Raman amplifiers achieve effective NF below 0 dB because gain is distributed along the transmission fiber — the signal is amplified before it is fully attenuated, effectively reducing the equivalent input loss compared to a discrete amplifier at the span end.
Cascade. For amplifiers in series with gains and noise factors (Friis formula):
The first amplifier in a chain dominates the overall noise figure if its gain is high. This is why pre-amplifiers immediately following the receiver are specified for low NF, while later amplifiers can tolerate higher NF.
NF directly limits the achievable OSNR of an amplified link — each amplifier in a span adds noise proportional to . Minimizing per-amplifier NF and selecting span lengths to maintain adequate per-stage gain is the central design problem for long-haul telecom.