SOA Semiconductor Optical Amplifier

Measurement Wavelength Range λ_P: min ：600； max ：1700 Measurement Wavelength Resolution λ_R: min ：±0.01 Measurement Wavelength Accuracy λ_A: min ：0.02

HYTS-ATS EDFA automatic test system is a precise, automated platform for fiber amplifiers. It automatically measures spectra, optical signal-to-noise ratio(OSNR), noise figure(NF), input/output optical power, and total power consumption. Integration with environmental-test equipment such as temperature chambers provides combined temperature/performance testing. Host software centrally controls optical switches, instruments, and chambers for efficient batch testing of single-channel or multichannel amplifiers, with channel expansion through optical switches. It supports high-reliability, high-consistency verification of aerospace products.

Wavelengths [Standard Version]: 2780±50nm Output Power [Standard Version]: 10mW-1W,>1W Signal Gain [Standard Version]: 10-20dB,>20dB

Efficient all-fiber amplification around 2800nm. The Amp 2800 mid-IR ultrafast fiber amplifier is a commercial erbium-doped fluoride-fiber amplifier with gain near 2800nm. Amp 2800 delivers watt-level power, diffraction-limited quality, and optical coupling efficiency above 20%, ideal for generating or amplifying mid-IR light. It supports mid-IR solid-state and semiconductor amplification, supercontinuum generation, and tunable ultrashort-pulse amplification. With ultrafast pumping, it generates watt-level tunable ultrafast output or high-energy supercontinuum spanning 2.6 to 4.2 µm. Strong gain near 3μm supports operation from CW to femtosecond pulses. Application example: mid-IR ultrafast amplifier and spectral converter.

Output Power [Nd Wavelength Band 461nm; Original Table “ Model ” Row :532-671nm]: ≤10W Input Power Range [Nd Wavelength Band 461nm; Original Table “ Model ” Row :532-671nm]: 1mm Beam quality M² [Nd Wavelength Band 461nm; Original Table “ Model ” Row :532-671nm]: M²≤1.2

Our single-frequency fiber amplifiers provide gain over broad wavelength ranges while preserving narrowband single-frequency signals. Optimized for high output from narrowband sources, they avoid triggering stimulated Brillouin scattering (SBS). They can work with second-harmonic generation (SHG) modules to efficiently convert NIR to visible light. Original main-parameter table (source header anomalies retained): Visible Fiber Amplifier 461-729nm | Nd Band 461nm | Yb Band 488-560nm | VRFA Series 550-765nm Model | 532-671nm | ≤4W | ≤4W Output Power | ≤10W | ≤10W | ≤10W Input Power Range | 1mm | 1mm | 1mm Beam Quality | M²≤1.2 | M²≤1.2 | M²≤1.2 Polarization Extinction Ratio | <0.5% | <0.5% | <0.5% Model | ER Band | Tm Band | RFA | RFA | RFA | RFA | RFA | EDFA Band | TDFA Band Model | 775-800nm | 813 and 832nm | 1100-1280nm | 1290-1360nm | 1370-1400nm | 1410-1525nm | 1600-1720nm | 1530-1590nm | 1730-195nm Output Power | ≤10W | ≤4W | ≤20W Air-cooled | ≤15W | ≤5W | ≤8W | ≤5W | ≤10W | ≤10W Input Power Range | 10-50mW | 10-50mW | 10-50mW | 10-50mW | 10-50mW | 10-50mW | 10-50mW | 10-50mW | 10-50mW Polarization Extinction Ratio | 20dB | 20dB | 20dB | 20dB | 20dB | 20dB | 20dB | 20dB | 20dB Beam Quality | M(2)<1.1 | M(2)<1.1 | M(2)<1.1 | M(2)<1.1 | M(2)<1.1 | M(2)<1.1 | M(2)<1.1 | M(2)<1.1 | M(2)<1.1