Broadband-Plasma Inspection System
Broadband-plasma inspection illuminates the wafer with a broad spectrum of light — using a plasma light source rather than a single laser wavelength — and captures how defects scatter or absorb across that whole spectrum at once, catching a wider range of defect types and sizes in a single pass than a single-wavelength laser-based inspection tool can.
A single laser wavelength is inherently blind to certain defect sizes and material combinations, which is exactly the gap broadband illumination closes. A defect's optical scattering signature depends on its size relative to the illuminating wavelength and its material's optical properties at that specific wavelength — a defect that scatters strongly at one wavelength might be nearly invisible at another, so a single-wavelength laser scanner can systematically under-detect certain defect populations. Spreading the illumination across a broad spectrum means some wavelength in that range is likely to interact strongly with almost any defect type, closing the blind spots a narrowband source leaves open.
The tradeoff is defect classification becomes more complex, since a signal that lights up strongly at one wavelength but weakly at another carries information a single-wavelength signal simply doesn't have. Broadband-plasma inspection systems have to process and interpret scattering data across multiple wavelength bands simultaneously rather than a single clean signal, which adds signal-processing complexity in exchange for catching the broader defect population a narrowband laser scanner would partially miss — a cost most production inspection flows accept given how much more complete the resulting defect coverage becomes.
Broadband-plasma inspection exists because no single wavelength of light interacts strongly with every possible defect a fab needs to catch, and spreading the illumination across a full spectrum is a more direct fix for that blind-spot problem than trying to guess the one best wavelength for every defect type in advance.