Suppress stray light at the surface level with ultra-thin, vacuum deposited black coatings applied directly to your optical components.
Acktar provides fully inorganic, vacuum deposited black coatings applied directly to customer parts or supplied as coated foils and films. Coatings are typically <5 µm thick, selectively masked, and qualified to absorb unwanted light across relevant wavelengths from UV through VIS, NIR, MWIR, and into FIR reducing reflections, scattering, and ghosting before they propagate through the system.
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What Problem Does This Solve?
Stray light is any light that reaches a detector or sensitive surface outside the intended optical path. It originates from surface reflections, micro-scattering, diffraction effects, and incomplete absorption inside optical assemblies. Even very low residual reflectance can measurably degrade system performance.
In real optical systems, stray light leads to:
- Loss of image contrast and dynamic range
- Reduced signal-to-noise ratio
- Ghost images and flare
- Measurement uncertainty in metrology and spectroscopy
- Unwanted thermal loading of detectors and nearby structures
The impact becomes more significant in systems involving:
- Broadband spectral operation (UV–IR)
- Grazing-incidence geometries and compact optical layouts
- High-sensitivity detectors and low-signal measurements
- Vacuum, cryogenic, or space environments
Stray-light mitigation is typically addressed through a combination of optical design, mechanical baffling, surface treatments, and, in some cases, electronic signal correction.
Paints, anodization, and polymer-based coatings can reduce reflections and are widely used in many applications. However, depending on the environment and wavelength range, they may exhibit:
- Higher residual reflectance
- Wavelength-dependent optical behavior
- Thickness buildup affecting fine geometries
- Surface instability under vacuum or thermal cycling
Mechanical baffles can block direct optical paths but do not eliminate surface reflections. Electronic correction methods can reduce visible artifacts after detection, but they do not prevent stray light from entering the optical path. For high-performance optical systems, controlling stray light at the surface level is often required in addition to mechanical and electronic strategies.
Acktar’s Approach to Stray Light Suppression
Acktar reduces stray light by qualifying absorption at the surface level using proprietary vacuum deposition processes. Fully inorganic coatings are deposited with controlled nano- and micro-scale morphology designed to trap incident light.
Key characteristics:
- Extremely low total hemispherical and specular reflectance
- Diffusive optical behavior that reduces ghosting
- Stable absorption across wide spectral bands
- Consistent performance over a broad range of angles of incidence
Because the coatings are typically <5 µm thick, they preserve sharp edges, apertures, pinholes, and fine geometries without dimensional buildup. All coatings are fully inorganic and qualified for low outgassing and long-term stability in demanding environments, including thermal vacuum, cryogenic operation, and space exposure.
In many systems, optimal performance is achieved by combining:
- Surface absorption (vacuum-deposited coatings)
- Mechanical baffling
- Optical layout optimization
- Electronic signal processing
Acktar’s contribution operates at the physical surface level—reducing unwanted optical energy before it propagates through the system.
Implementation Approaches
Acktar supports two complementary implementation paths:
- Direct Coating on Customer Components
Customer furnished parts are coated at Acktar’s facilities with selective masking, ensuring only optically relevant areas are coated while functional surfaces remain untouched. - Coated Foils, Films, and Sheets
Acktar supplies pre-coated foils, films, and sheets that can be integrated into optical assemblies, applied to housings, or used for internal baffling where direct coating is not practical.
Recommended Coatings – Direct Coating on Parts
| Coating Family | Typical Spectral Range | Key Optical Behavior | Typical Applications | Environmental Capability |
| Magic Black™ | EUV – UV – VIS | Extreme absorption, ultra-low reflectance | EUV optics, UV instruments | Vacuum, cryogenic, space-qualified |
| Vacuum Black™ | EUV – NIR | Ultra-low specular and hemispherical reflectance | Optical baffles, metrology tools | Vacuum, thermal cycling |
| Fractal Black™ | VIS – IR (to FIR) | Diffusive ultra-black absorption | Imaging systems, spectrometers | Cryogenic to high temperature |
| Core Black™ | EUV – NIR | Ultra-flat, particle-free, diffusive | Wafer chucks, precision mounts | Vacuum, ESD-safe, ultra-clean |
Recommended Coatings – Foils, Films, and Sheets
| Product | Form Factor | Spectral Range | Key Optical Behavior | Typical Applications |
| Hexa-Black™ | Absorbing sheets / panels | UV – MWIR | Lowest reflectance at grazing angles (40°–88° AOI) | Grazing-angle baffles, beam tunnels |
| Metal Velvet™ | Coated aluminum foils | UV – IR | Highly diffusive absorption | Light traps, internal housings |
| Fractal Black™ on Polyimide | Flexible films | UV – MWIR | Diffusive absorption, flexible | Internal baffling, space payloads |
| Fractal Black™ on Copper | Flexible copper foils | VIS – IR | Absorption + high thermal conductivity | Opto-thermal assemblies |
Technical Performance
- Spectral coverage: EUV/UV through VIS, NIR, MWIR, and FIR (coating-dependent)
- Total hemispherical reflectance: typically <1.3%, reaching <1% at selected wavelengths
- Specular reflectance: near-zero
- Emissivity (3–30 µm): typically >0.85 (product dependent)
- Angular performance: stable absorption at normal and grazing incidence (product dependent)
- Coating thickness: typically <5 µm
- Outgassing: qualified for vacuum and space applications (coating/product dependent)
- Environmental compatibility: vacuum, thermal vacuum, cryogenic operation, atomic oxygen exposure (product dependent)
Performance is validated through qualification testing including thermal cycling, thermal vacuum cycling, cryogenic exposure, adhesion testing, and reflectance stability after environmental stress.
Typical Applications
- Internal optical baffles and light traps
- Precision apertures, pinholes, diaphragms, and stops
- Imaging systems, cameras, and machine-vision assemblies
- Telescopes, spectrometers, and scientific instruments
- Laser beam dumps and absorbers
- Semiconductor inspection and metrology tools
- Spaceborne optical payloads and sensors
Integration & Compatibility
- Substrates: aluminum, copper, stainless steel, titanium, tungsten, magnesium, molybdenum, nickel, Invar, Kovar, ceramics, glass, polymers, polyimide
- Formats: direct coating on parts, foils, films, sheets, rolls, die-cuts, patterned components
- Geometries: complex 3D parts, fine apertures, sharp edges, thin structures
- Manufacturing routes: customer-furnished parts, coating of patterned sheets, customer patterning of coated materials, or full turnkey manufacturing
- Cleanliness: cleanroom-compatible handling and packaging
- Outgassing / UHV: fully inorganic coatings qualified for vacuum use; low-outgassing performance available for space, thermal-vacuum, and UHV environments (coating/product dependent)
Mission Proven Results
Acktar coatings are deployed in operational systems across space, semiconductor, metrology, laser, and scientific instrumentation markets, delivering measurable improvements in contrast, signal-to-noise ratio, and long term optical stability.
Related Solutions
- Thermal Control and Emissivity Management
- Laser Light Management
- High-Performance Optical Coatings