Dense spiral coil of glowing optical fibre against deep black background with blue and amber light gradients, intense infrared glow at fibre tip suggesting high-power photonics operation.
Woodrow Scientific
High-Power Fiber Amplifier - Custom EDFA by WSL
High-power fiber amplifier built to spec — up to 200 W average, 100 kW peak power, eye-safe 1550 nm MOPA platform. CE and UKCA certified, built in Southampton.

Why Architecture and Application Must Align

A high-power fibre amplifier boosts an optical signal to the levels a demanding application requires, entirely within the optical domain. LiDAR, free-space optical communications, defence, and sensing all depend on this capability.

The established architecture is MOPA: a seed laser feeding multi-stage amplification through erbium-doped fibre, across the 1530–1625 nm window — the minimum-loss band of silica fibre.

Operating band, output power, pulse regime, and integration envelope all shift what an amplifier delivers. A catalogue part fixes those variables for you. For demanding work, the amplifier must be built around the application — not the other way round.

Isometric schematic of MOPA fibre amplifier chain: seed laser on left feeding three erbium-doped fibre amplifier stages with pump injection, progressing to high-power output stage on right. Electric blue signal and pump lines show signal flow. Operating window 1530–1625 nm labeled.
Power Specifications

Power Performance Specifications

Every figure below is a configurable performance ceiling, built to the client's requirement. Average power, pulse energy and peak power are all scalable per project — these are not fixed SKU specifications but the current expression of what WSL engineers to order.

Intense electric blue fiber laser beam emerging from metallic fiber tip against dark navy technical background, with ionization effects visible around the high-energy beam path.

Average Power: Up to 200 W or More

Builds to 200 W or more — the highest average power commercially available.

Oscilloscope display with sharp electric blue optical pulse waveform centered on dark screen, showing high-energy peak against dark technical background with grid pattern.

Pulse Energy: Above 10 mJ

Pulse energies above 10 mJ, specified and configured per project to the application's requirement.

Towering electric blue optical waveform spike rising sharply from baseline against dark navy background, representing ultra-high peak power pulse above 100 kW with glowing cyan halo suggesting laser energy intensity.

Peak Power: Above 100 kW

Peak powers above 100 kW, configurable per project to meet the application's demands.

Precision power slider control with polished metal handle positioned at 75% output, mounted on light grey panel against clean technical background with subtle grid pattern.

Full Output Control: 0 to 100%

Output continuously tunable from 0 to 100% of rated power, no fixed steps.

Technician in navy coveralls assembling a custom fibre amplifier module on a precision workbench in a bright, clean workshop with cool-toned lighting.

Built to Your Power Requirement

Every unit engineered to the client's specification. Requirements beyond published figures are assessed directly.

Configurable Parameters: Engineered to Your Specification

Operating Band

C-band, L-band, or Both

The Custom EDFA operates across the C-band (1530–1565 nm), the L-band (1565–1625 nm), or both simultaneously — delivered through a single cable from a single amplifier, with no second source required.

Band selection is specified per project. Whether your optical architecture demands C-band, L-band, or dual C+L coverage, the amplifier is built to match it — not the other way around.

Wavelength band diagram showing the 1530–1625 nm erbium window divided into C-band (1530–1565 nm) and L-band (1565–1625 nm) regions on a horizontal spectrum bar with fiber optic cable icon at output indicating dual-band delivery.
Power & Pulse

Power Built to Spec

Output power, pulse energy and peak power are all configured per project. Builds range from low-power units to 200 W or more average power, with pulse energies above 10 mJ and peak powers above 100 kW — the figures established in the preceding section are targets, not fixed ceilings.

Output is continuously tunable from 0 to 100% of rated power. Submit your requirements to discuss what the build looks like for your application.

3D power envelope diagram with three performance axes: average power (200 W+), pulse energy (10 mJ+), and peak power (100 kW+), with central tuning slider marked 0–100% of rated output.
Pulse Regime & Cooling

Regime and Cooling

The pulse regime is specified per project: CW, short-pulse (e.g. 100–500 ns), or a custom configuration. The amplifier is built to the temporal profile your application requires.

Air-cooled as standard — no chiller or coolant loop required, which simplifies integration into your system. Water cooling is available as an option for builds where it is preferred.

Split technical diagram: left panel shows pulse regime waveforms for CW, short-pulse (100–500 ns), and custom configurations on a time axis; right panel compares air-cooled unit with fan icon to water-cooled option with coolant loop icon.
Cable & Form Factor

Cable and Form Factor

Delivery cable length and fibre termination are specified per project, so the amplifier connects directly to your system without adaptation or compromise.

The form factor and integration envelope are custom to each build. There is no fixed chassis to design around — the amplifier is sized and shaped to fit your system, whether that is a rack, a payload, or a bespoke housing.

Compact custom erbium-doped fibre amplifier module with Woodrow Scientific branding on a light optical bench, delivery cable routed neatly to a fibre termination point in the background.
Firmware & Platform

Firmware and Platform

Control firmware and communication standards are custom per project. The amplifier is configured to speak your system's protocol, removing the integration overhead of bridging incompatible interfaces.

The fixed foundation: erbium-doped fibre gain medium, MOPA architecture, and a 1530–1625 nm wavelength window. These are the stable platform on which all configurable parameters sit — the physics and architecture that make the performance possible.

Layered stack diagram showing fixed technical foundation of Custom EDFA with erbium-doped fibre, MOPA architecture, and 1530–1625 nm wavelength window as immovable base blocks, and configurable layers above for power output, pulse regime, cooling, and control firmware.

The 1550 nm Erbium-Fibre Platform

Eye-Safe Wavelength

Why 1550 nm Is Safer

Wavelengths above 1400 nm are absorbed by the cornea and lens of the eye rather than transmitted to the retina — the tissue most vulnerable to permanent laser damage. At 1064 nm, collimated light reaches the retina and is focused to an intense spot; at 1550 nm, it does not. The Laser Institute of America confirms this distinction: 1400 nm marks the boundary of the retinal hazard region.

The result is a materially higher maximum permissible exposure at 1550 nm. WSL's Custom EDFA operates in this window, with reduced-hazard-zone builds available for safety-critical deployments.

Cross-section diagram of human eye showing laser beam paths at two wavelengths: 1064 nm converging to focal point at retina labeled retinal hazard region; 1550 nm absorbed at cornea and lens. Horizontal line marks 1400 nm absorption threshold.
Safety Classification

Higher MPE, Smaller Hazard Zone

IEC 60825-1 is the international standard governing laser product safety classification and maximum permissible exposure (MPE). Because the MPE at 1550 nm is materially higher than at 1064 nm — a direct consequence of the retinal hazard boundary at 1400 nm — a 1550 nm system can operate at a given output power with a smaller nominal ocular hazard distance than an equivalent 1064 nm system. In practical terms: higher permissible operating power at a given hazard zone size, or a reduced hazard zone at equivalent power. Both translate to simpler site safety planning and easier compliance sign-off.

Concentric laser hazard zone diagram with 1550 nm inner zone and 1064 nm outer zone, labeled with safety standard IEC 60825-1.
Reduced Hazard Zone

Built for Simpler Site Compliance

WSL offers reduced-hazard-zone builds of the Custom EDFA — a direct procurement and site-planning benefit for buyers operating in safety-conscious environments. A smaller exclusion zone means less floor area to control, fewer access restrictions, and a more straightforward path through safety sign-off and regulatory review.

For integration teams working within constrained facilities or tight compliance timelines, this simplifies the process of bringing a high-power fibre amplifier into service. The specific hazard zone achieved depends on power level and configuration; WSL's engineering team works through the details with each customer at specification stage.

Compact EDFA fibre amplifier system on a laboratory bench in a bright technical facility, with neatly routed optical cables and minimal footprint.
Why This Window

Where Modern Photonics Converges

Three physics-driven reasons have made 1530–1625 nm the dominant window for high-power photonics. First, silica fibre reaches its loss minimum in this region — IEEE sources confirm standard single-mode fibre achieves around 0.18–0.20 dB/km near 1550 nm, enabling long-reach transmission. Second, 1550 nm sits within a well-established atmospheric transmission window, making it the standard choice for free-space optical links. Third, the global telecom industry built its C- and L-band component ecosystem — detectors, connectors, modulators, test equipment — around this window, so system integration draws on a deep, mature supply chain rather than bespoke parts.

NIR spectrum graph showing wavelength range 800–1800 nm with 1530–1625 nm highlighted in electric blue. C-band and L-band marked as sub-regions. Vertical reference line at 1550 nm indicates minimum fibre loss point. Two annotation labels identify minimum fibre loss (~0.18–0.20 dB/km) and atmospheric transmission window.
C+L Dual Band

Both Bands, One Cable

The Custom EDFA delivers both C-band (1530–1565 nm) and L-band (1565–1625 nm) from a single amplifier through a single cable. No second amplifier source is required, no second cable run, and no additional integration overhead to combine outputs from separate units.

For system architects, this is a straightforward engineering advantage: one procurement item, one interface, one support relationship. The full 1530–1625 nm window is available from a single point in the signal chain, simplifying both the bill of materials and the integration design.

Technical diagram of dual-band fiber amplifier showing central amplifier unit with C-band (1530–1565 nm) and L-band (1565–1625 nm) output paths converging into single cable output, labeled with electric blue connector lines on light background.
Applications

Applications: Where the Custom EDFA Is Deployed

The Custom EDFA serves demanding application domains where high-power, eye-safe erbium-fibre amplification is the enabling technology — engineered to each programme's specific requirements.

Nighttime aerial LiDAR detection scene with pulsed electric blue laser beam sweeping across dark landscape, sensor unit in foreground, and glowing teal point-cloud terrain map on right showing real-time 1550 nm range data acquisition.

LiDAR: Extended Range at Eye-Safe Power

Eye-safe 1550 nm permits higher pulse power than 905 nm sources, extending detection range. The MOPA architecture delivers short, high-peak-power pulses LiDAR ranging requires.

Ground-based optical terminal with precision telescope dish pointed skyward, vivid electric blue infrared laser beam rising toward sky against deep blue twilight backdrop, representing free-space optical communications uplink at 1550 nm.

Free-Space Optical Communications (FSOC)

1550 nm sits in an atmospheric transmission window, compatible with telecom-grade components. High average power supports link budgets for ground-station uplink and beacon amplification.

Compact fibre amplifier module mounted in ruggedised equipment enclosure with optical cables routed to directed-energy aperture assembly in military integration bay

Defence and Directed-Energy Research

High average power, pulse energy, and peak power in the eye-safe band meet defence programme requirements. Configurable pulse regime and form factor enable platform integration.

Quantum photonics laboratory optical bench with single-mode fiber spools, beamsplitters, and photon-counting detectors arranged on precision-engineered optical table, illuminated by faint infrared glow at 1550 nm.

Quantum Sensing and Communications

The C-band 1550 nm window coincides with minimum loss in silica fibre — the established wavelength for QKD and quantum sensing over fibre infrastructure.

Cross-section of buried fibre optic cable with acoustic wavefronts propagating downward from surface and DAS interrogator unit at left emitting pulsed laser signal along cable.

Distributed Acoustic Sensing and Fibre Sensing

EDFA pulse amplification is the standard interrogator architecture for DAS systems at 1550 nm. High peak power extends the sensing range along the fibre.

Fibre-coupled laser amplifier module mounted in stainless steel instrument rack with precision power control interface, digital readout display, and spectral monitoring indicators; adjacent amplifier module visible in background establishing multi-unit system.

Remote Sensing and Scientific Instrumentation

Research platforms and atmospheric instruments require precise power control and spectral stability. Full 0-100% output control and configurable pulse regime serve these requirements.

Engineering workspace showing a custom fibre amplifier module integrated into an OEM laser system chassis, with fibre connectors, control firmware interface on a display panel, and structured cable management.

OEM Laser System Integration

The Custom EDFA serves as the optical engine for OEM laser builds, configured to the integrator's form factor, firmware, and communication standards.

Ready to Specify Your High-Power Fibre Amplifier?

Download the EDF100 datasheet for concrete performance figures, or speak directly with WSL's engineering team about your application requirements and custom specification.

Coiled optical fibre glowing with intense infrared light against a near-black technical backdrop with subtle beam propagation effects and faint geometric grid pattern

Built by People Who Know It

The Birthplace

Where the EDFA Was Born

The erbium-doped fibre amplifier was first demonstrated in 1987 by researchers at the University of Southampton, according to IEEE. WSL is based in Southampton and works closely with the people who pioneered that technology.

This is not decorative geography. It is direct intellectual lineage — the same institution, the same field, the same city where the high-power fibre amplifier as a discipline began.

Coiled erbium-doped optical fiber glowing with faint electric blue infrared luminescence against dark navy laboratory backdrop with subtle Southampton coordinate grid pattern.
The Team

Deep Expertise, From the Source

WSL was founded in 2012 by a fibre-laser specialist holding a PhD from Southampton's Optoelectronics Research Centre, with 25+ years in the field. The team works closely with the people who pioneered erbium-fibre amplification.

Across a team of more than 20 specialists, WSL carries over 200 years of combined engineering experience — depth that bears directly on how each amplifier is specified, built, and supported.

Senior engineer in lab coat examining fibre-optic assembly under stereo microscope in bright technical workspace, demonstrating hands-on expertise with high-power fiber amplifier components.
In-House Build

Designed, Built, and Supported Here

Every Custom EDFA is engineered, assembled, qualified, and supported by the same WSL team in Southampton. When an integration issue arises, the engineers who answer are the engineers who built the unit.

Many EDFA suppliers are resellers or importers rather than manufacturers. With WSL, the engineering relationship sits with the team you deal with directly — not with an overseas manufacturer behind the supply chain.

Precision optical amplifier module with Woodrow Scientific branding on a bright laboratory workbench, with an engineer in navy coveralls adjusting fibre optic cable connections while test equipment sits nearby.
Patents

10 Patents and Counting

WSL holds 10 patents and counting — a direct measure of continuous, in-house innovation on the technology rather than resale of an established product.

The patent portfolio reflects the same engineering model that underpins every build: proprietary development, owned and controlled by the team that designs and manufactures the amplifier.

Photorealistic fibre amplifier unit with dark navy chassis on light technical background, electric blue bordered badge overlay reading '10 PATENTS and counting' positioned upper-right
Worldwide Supply

Direct from Southampton, Anywhere

Buyers in any country order direct from WSL in Southampton — no distributor layer, no intermediary, and a direct engineering relationship from first contact through to delivery and integration support.

Three-dimensional globe with Southampton, UK marked by a bright electric blue glowing node, radiating thin connection lines to destinations across North America, Europe, Asia, and Australia on a dark navy technical background.

CE and UKCA Certified for EU and GB Markets

The Custom EDFA carries both CE marking and UKCA marking. Buyers placing the product on the EEA market or the GB market can proceed without a re-certification gap — both marks are held simultaneously.

WSL's engineering team supports every buyer from initial specification through to deployment and integration.

Woodrow Scientific Custom EDFA amplifier unit on light grey surface with CE and UKCA certification badges positioned above the device.

Frequently Asked Questions

Technical and procurement questions about the Custom EDFA, answered directly.

The Custom EDFA is quoted per project, not selected from a catalogue. Submit your requirements — operating band, output power, pulse regime, cooling preference, form factor, and firmware or communication standards — and WSL's engineering team evaluates the specification and responds with a tailored proposal. There is no fixed SKU to configure around; the amplifier is built to your application.

Yes. The specifications and applications shown on this page represent what WSL has built so far, not the boundary of what it can engineer. A requirement beyond the published figures — a different environment, an unusual power level, a non-standard form factor, a bespoke pulse regime — is assessed directly with the client by WSL's engineers. The right approach is to submit the requirement and discuss it; WSL does not rule requirements out in advance.

Yes. The 1530–1625 nm erbium-fibre window operates above the 1400 nm threshold, above which radiation is absorbed by the anterior ocular media — the cornea and lens — rather than reaching the retina. ICNIRP's laser guidelines confirm that 400–1400 nm is the retinal hazard region; wavelengths beyond it do not contribute to retinal exposure. The Custom EDFA therefore carries a materially higher eye-damage threshold than 1064 nm sources, and WSL offers reduced-hazard-zone builds for buyers where site safety classification is a procurement consideration.

Yes. Buyers in any country order direct from WSL in Southampton. There is no distributor layer — the buyer works directly with WSL's engineering team from first contact through to delivery and integration support.

A fiber amplifier boosts the power of an optical signal entirely in the optical domain, without converting it to electrical form. According to IEEE, an erbium-doped fiber amplifier (EDFA) operates by pumping a length of erbium-doped silica fiber with a laser diode at 980 nm or 1480 nm, exciting the erbium ions; incoming signal photons then stimulate those ions to emit coherent photons at the same wavelength, producing gain. In a MOPA architecture, a seed laser provides the signal and one or more amplifier stages raise it to the required output power. The standard operating window for erbium-doped amplifiers is 1530–1625 nm — covering the C-band (1530–1565 nm) and L-band (1565–1625 nm) — which coincides with the minimum-loss transmission window of silica fiber.

In the context of erbium-fibre amplifiers, high power means average output well above the typical commercial ceiling. Most EDFA builds operate at modest average powers; a high-power fibre amplifier is one engineered to deliver significantly greater output for demanding applications such as LiDAR, free-space optical communications, defence, and distributed sensing. WSL's Custom EDFA scales from low-power builds to 200 W or more average power, with pulse energies above 10 mJ and peak powers above 100 kW. Output is continuously tunable from 0 to 100% of rated power.