Description

OPTOMAN PP-UVFS-25.4-6.35-LLM214 is a high-performance GTI dispersive mirror engineered for precise negative Group Delay Dispersion (GDD) control in ultrafast laser systems. Featuring an IBS dielectric coating on UV fused silica substrate, this mirror delivers high reflectivity above 99.9% across the 980–1080 nm wavelength range while providing a controlled GDD value of -350 fs² ±120 fs² at a 5° angle of incidence.

Designed for applications requiring accurate pulse compression and dispersion management, this 25.4 mm diameter mirror supports stable operation in femtosecond and picosecond laser oscillators, amplifiers, and pulse conditioning setups. Its low absorption characteristics and high optical quality make it suitable for demanding high-power ultrafast photonics applications.

PP-UVFS-25.4-6.35-LLM214 GTI Dispersive Mirror for Ultrafast Lasers

Specifications

Substrate Material: UVFS
Diameter: 25.4 mm
Thickness: 6.35 mm
Clear Aperture (CA): 90 %
Surface Quality, S1 (scratch-dig): 10-5
Surface Quality, S2 (scratch-dig): Commercial Polish
Surface Flatness, S1 (@ 633nm Over CA Or Per Manufacturer): <= Lambda/10
Wedge, S1: 0.17 arcmin
Optimized AOI: 5 – 5 deg
Average Reflectance (@ Peak Wavelength Range, Optimized AOI): 99.9 %
Average GDD (@ Peak Wavelength Range, Optimized AOI): 350 fs^2
Manufacturer Part Number (MPN): PP-UVFS-25.4-6.35-LLM214
FindLight SKU: FL-24581

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Features

  • IBS-coated GTI dispersive mirror for ultrafast laser applications
  • Provides negative Group Delay Dispersion (GDD): -350 fs² ±120 fs²
  • Optimized for 980–1080 nm wavelength operation
  • Designed for Yb:YAG laser systems at approximately 1030 nm
  • High reflectivity: HR >99.9% at 980–1080 nm
  • UV fused silica substrate for excellent thermal and optical stability
  • Low absorption: <20 ppm at 1064 nm
  • Surface quality: 10-5 scratch-dig
  • Surface flatness: <λ/10 at 633 nm over 10 mm diameter area
  • Precision 5° angle of incidence operation
  • 25.4 mm diameter with 6.35 mm thickness standard format

Applications

  • Femtosecond laser pulse compression systems
  • Picosecond and ultrafast laser oscillators
  • Yb:YAG laser dispersion compensation
  • Chirped pulse amplification (CPA) systems
  • Ultrafast amplifier cavities
  • Precision optical delay and pulse shaping systems
  • High-power laser research and development platforms
  • Nonlinear optics and advanced photonics experiments

Export & Trade Information

ECCN: EAR99
HTS Code: 9001.90.6000
Estimated US Tariff: 10%

Importing, tariffs & codes (Quick Guide) →

Frequently Asked Questions

What type of optical component is the OPTOMAN PP-UVFS-25.4-6.35-LLM214?
The OPTOMAN PP-UVFS-25.4-6.35-LLM214 is a GTI dispersive mirror designed to introduce controlled negative Group Delay Dispersion (GDD) into ultrafast laser systems. It uses interference effects inside the dielectric coating structure to manage pulse dispersion while maintaining high reflectivity.
What wavelength range is the PP-UVFS-25.4-6.35-LLM214 optimized for?
This GTI mirror is optimized for operation from 980 nm to 1080 nm, making it suitable for near-infrared ultrafast laser systems, particularly Yb-based laser sources operating around 1030 nm.
What is the GDD value of this OPTOMAN dispersive mirror?
The PP-UVFS-25.4-6.35-LLM214 provides a negative Group Delay Dispersion value of -350 fs² ±120 fs² at 980–1080 nm with a 5° angle of incidence.
What substrate material is used for this GTI mirror?
The mirror is manufactured using UV fused silica (Corning 7980 0F) substrate material, offering excellent transmission properties, low thermal expansion, and reliable performance in demanding laser environments.
Which laser systems can benefit from using the PP-UVFS-25.4-6.35-LLM214 mirror?
This mirror is ideal for femtosecond and picosecond laser systems that require precise dispersion compensation, including Yb:YAG lasers, ultrafast oscillators, amplifiers, and pulse compression setups where stable pulse duration control is essential.

Got more questions? Use the inquiry form to ask the supplier directly.

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