KLA

Darkfield inspection works by directing a laser or broadband light source onto the wafer surface at an oblique angle. The specular reflection is blocked from reaching the detector, while light scattered by particles, pits, scratches, or pattern anomalies is collected and imaged. The system uses multiple collection channels, typically including forward-scatter and back-scatter optics, to capture different defect signatures.
The collected scatter signals are converted into electrical signals and processed by the system's image-analysis software. Defects are classified by size, type, and location using algorithms trained on reference die or golden images. The tool can operate in both brightfield and darkfield modes depending on configuration, but the Altair series is dedicated to darkfield detection.
The tools sit between front-end-of-line and back-end-of-line processing, often as part of a defect-review workflow. Wafers rejected by darkfield inspection may be sent to review scanning electron microscopes or atomic-force microscopes for further analysis.
Common applications include incoming substrate qualification, post-chemical-mechanical planarization residue checks, defect-density monitoring after dielectric deposition, and post-etch inspection. The high throughput of automated darkfield systems makes them suitable for volume production environments.
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Brightfield inspection captures directly reflected light, making it suitable for imaging fine pattern features and subtle reflectivity changes. Darkfield inspection captures only scattered light, providing higher sensitivity to discrete particles and small topographical defects on smooth surfaces.
Throughput varies widely depending on the machine design, scanning speed, and defect sensitivity requirements. High-volume manufacturing systems are designed to inspect wafers in minutes per wafer for standard recipes, balancing speed with resolution.
Yes, darkfield inspection is used for both unpatterned and patterned wafers. On patterned wafers, the technique is especially useful for detecting defects in low-topography structures or on film surfaces where pattern contrast is minimal.
Key factors include the angle and polarization of illumination, the numerical aperture of the collection optics, the wavelength of light, and the signal-to-noise ratio of the detector. System calibration and the reflectivity of the wafer surface also play important roles.
The following facts about the Altair 8920 Darkfield are absent from this record as of this revision. First-hand knowledge or a citation closes a gap; every submission is reviewed before publication.
No publicly documented production dates or lifecycle milestones (introduction, end of production, EOL) for the Altair 8920 Darkfield are on record.
Answerable by: OEM historical records or a trade-press announcement
No publicly documented variants, configuration options, or revision breakpoints of the Altair 8920 Darkfield are on record.
Answerable by: an OEM product catalog or an engineer who ordered or specified the tool
The control-system platform and OS era of the Altair 8920 Darkfield are not on record.
Answerable by: an engineer who operated it or OEM installation records
No publicly documented failure modes or field errata for the Altair 8920 Darkfield are on record.
Answerable by: a field service engineer, process engineer, or maintenance technician
The process node or technology generation of the Altair 8920 Darkfield is not on record.
Answerable by: an OEM datasheet or a fab qualification report
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Last updated Oct 11, 2026.
The KLA .204 PSL Wafer is an 8-inch NIST-traceable reference wafer compatible with Surfscan 6xy0 and Sp1 particle counters.
KLA .496 PSL Wafer is an 8-inch NIST traceable wafer stated to be capable on Surfscan 6xy0 and SP1.
The KLA .498 PSL Wafer is a NIST traceable reference wafer.