Super Low Loss Flat Mirror

① Dimension D=φ3-φ25mm (tolerance ±0.1),H=3-8mm D:H > 4:1 (tolerance ±0.5)
D=φ26-φ100mm (tolerance ±0.1),H=6-25mm D:H > 5:1 (tolerance ±0.5)
② Coating area size: conventional size D12.7, coating area size 7.5; D25 coating area size 10, other coating area size can be customized
③ Surface accuracy: λ/ 10@632.8nm
④ Parallel error: <10"
⑤ Roughness: Ra0.12nm (Zygo profilometer) test area 173*173um full frequency measurement
⑥Coating requirement: wavelength 420nm-3000nm, reflection ≥99.999%, loss 2-3ppm, transmission 3-5ppm
Back anti-reflection;
⑦ Material: ULE, fused silica, single crystal silicon, sapphire;
Note: The specific indicators are not limited to the above scope, and can be customized according to user's needs.
Application:Laser gyro, high power laser, super stable laser, high precision optical detection
Product Description

Super Low Loss Flat Mirror: Precision Optics for Extreme Environments

When every photon counts, our Super Low Loss Flat Mirror delivers unmatched performance in mission-critical applications. Designed for aerospace, defense, and high-power laser systems, these mirrors combine <0.1% absorption rates with >99.999% reflectivity to minimize signal loss under thermal stress, radiation, and mechanical shock.

Why Choose Our Ultra-Low Loss Mirrors?

Military-Grade Durability

  • Thermal Stability: Operate seamlessly from -270°C to +300°C, enduring cryogenic chambers and industrial heat without structural shifts, critical for quantum research and aerospace sensors where temperature extremes would warp standard optics, preserving alignment in deep-space probes or ultra-cold labs.​
  • Radiation Resistance: Proven performance in LEO/MEO satellite orbits, withstanding proton/electron flux that degrades conventional mirrors, ensuring consistent reflectivity for communication links and Earth-observation systems, vital for missions requiring long-term reliability in harsh space environments.​
  • Surface Precision: λ/10 flatness & <0.5 nm roughness for zero wavefront distortion, eliminating light scattering in high-resolution imaging and laser interferometry, ideal for semiconductor metrology and astronomy telescopes where even minor irregularities would compromise data accuracy or image clarity.​

Custom-Built Performance

  • Material Options: ULE, fused silica, or sapphire substrates—ULE for extreme thermal stability, fused silica for high-power laser resilience, sapphire for 9 Mohs hardness, enabling tailored solutions for quantum labs, industrial lasers, or aerospace sensors based on specific environmental demands.​
  • Coating Flexibility: 420nm-3000nm wavelength optimization, from visible to near-infrared, enhancing performance in hyperspectral imaging and laser communication, ensuring maximum reflectivity at target wavelengths to minimize signal loss in satellite links or precision spectroscopy setups.​
  • Compact Sizes: From φ3mm to φ100mm with anti-reflective backing, fitting into miniaturized sensors and large optical arrays alike, ideal for drone-mounted LIDAR and ground-based telescopes, balancing space efficiency with optical performance in diverse applications.

Trusted by Industry Leaders

"Reduced laser system downtime by 40% in variable thermal zones." – Aerospace OEM

Technical Specifications

Parameter Specification
Dimensions Dimension D=φ3-φ25mm (tolerance ±0.1),H=3-8mm D:H > 4:1 (tolerance ±0.5)
D=φ26-φ100mm (tolerance ±0.1),H=6-25mm D:H > 5:1 (tolerance ±0.5)
Coating Area Customizable (standard: D12.7mm, 7.5mm area; D25mm, 10mm area)
Surface Accuracy λ/10 @ 632.8nm
Parallel Error <10"
Roughness Ra0.12nm (Zygo profilometer) test area 173*173um full frequency measurement
Reflectivity ≥99.999% (420nm-3000nm)
Loss 2-3ppm
Transmission 3-5ppm
Materials ULE, fused silica, single crystal silicon, sapphire

Note: Specifications can be customized to meet your unique requirements.

Built for Critical Applications

  • Satellite Communications: Ensure uninterrupted signal integrity in harsh orbital environments with Super Low Loss Flat Mirror that withstand 500+ thermal cycles, leveraging ULE’s stability and radiation resistance to maintain >99.9% reflectivity, critical for GEO/LEO links where temperature swings and radiation would disrupt data transmission.​
  • High-Power Lasers: Handle >5kW/cm² continuous-wave loads without coating degradation – ideal for lidar and industrial cutting systems, using fused silica substrates and optimized coatings to resist thermal damage, ensuring consistent beam quality in high-stakes manufacturing and remote sensing operations.​
  • Surveillance & Reconnaissance: Maintain optical clarity in desert heat (-50°C to +80°C operational range) and 98% humidity, with sapphire’s hardness and moisture-resistant coatings preventing fogging or scratching, vital for reliable imaging in extreme climates where environmental stress would impair standard optics.

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Rigorous Quality Assurance

Every ultra-low loss mirror undergoes:

1. Interferometric surface analysis

2. 72-hour salt fog corrosion testing

3. Laser damage threshold validation

4. 100% defect inspection (0 scratches/pits in critical areas)

Flexible Ordering Options

Prototype Orders

  • 2-4 week lead time
  • Free performance simulation report

Volume Discounts

  • 10-25% savings on 100+ unit orders
  • Dedicated batch tracking & QA documentation

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FAQs

Q: How do your Super Low Loss Flat Mirror handle rocket launch vibrations?

A: All mounts are designed to MIL-S-901D specs, absorbing 15G RMS shock without alignment shift.

Q: Can I get anti-static coatings for dusty environments?

A: Yes – our proprietary ITO coatings reduce particle adhesion by 70%.

Q: What’s the lead time for φ50mm custom mirrors?

A: 6 weeks standard, 4 weeks expedited (+15% fee).

Ready to Upgrade Your Optical System?

Includes coating analysis report and integration guide

Contact Our Engineers Today 📧 xachaona@163.com about Super Low Loss Flat Mirror.​​​​​​​

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