Absorption Capabilities

Absorption is the tiny fraction of laser light an optical component converts into heat. Measured in parts per million (ppm), it is easy to overlook, yet it drives thermal lensing, focal shift, beam distortion, and coating failure in high-power laser systems.

Every ppm counts: the less a coating absorbs, the less it heats up and the more stable the laser system stays. OPTOMAN’s dense ion beam sputtered (IBS) coatings, made from ultra-high-purity materials, keep absorption to a minimum – so the beam stays unchanged at full power, hour after hour. 

ABSORPTION MEASUREMENTS

ABSORPTION MEASUREMENTS AND REPORTS

AR
HR
HR+HT
POL
Wavelength, nm Substrate material Measurement wavelength, nm AOI, degPolarization L-scan max, ppm Time scan, ppmT-scan avg, ppm Report
343BBO355 2 P 486 450 163 Download
980-1080 UVFS 1070 2 P 1.32 1.38 1.13 Download
1070IRFS 1070 2 P 0.1230.1 0.113 Download
1055-1080UVFS10702 P 1.250.85 0.9 Download
1064UVFS1070 2 P 1.61.75 1.635 Download
1065-1075 IRFS1070 2 P 0.0910.1 0.076 Download
Wavelength, nm Substrate material Measurement wavelength, nm Measurement wavelength, nm Polarization L-scan max, ppm Time scan, ppmT-scan avg, ppm Report
337-349 UVFS 355 45S 9590 82 Download
343 UVFS 355 45 S 51.3 50 44.4Download
980-1080 UVFS 1070 2 P16.0516.216.21Download
1010-1050UVFS1064 45 P0.5–1.2 0.5–1 0.5–1 Download
1030 + 630-660 UVFS1064 0 P0.40.60.5 Download
1030 + 650-660 UVFS 1070 45 S 0.7450.750.735Download
1030 + 1060-1100 UVFS1070 45 P 0.740.80.61 Download
1030 + 1064 UVFS1070 2 P 3.57 3.65 3.672Download
Wavelength, nm Substrate materialMeasurement wavelength, nm AOI, degPolarization L-scan max, ppm Time scan, ppm Time scan, ppm Report
355 + 532 +1064 UVFS 355 45 S 76.7 85 85 Download
970-990 + 1015-1045 UVFS 10702 P 1.52 1.62 1.619 Download
1035-1075 + 1550 + 915 + 808 UVFS 1070 45P 1.61.41.57Download
Wavelength, nm Substrate materialMeasurement wavelength, nm AOI, deg Polarization L-scan max, ppm Time scan, ppm T-scan avg, ppm Report
1015-1045UVFS107060 P 4.1244.04 Download
1020-1040UVFS1070 49 S2.1 2.22.16Download
1020-1040UVFS107049 P8.7 8.6 8.7 Download
Absorption Evaluation

HOW ABSORPTION DEPENDS ON WAVELENGTH

Between the near-infrared around 1 µm and its third harmonic in the UV, absorption differs by orders of magnitude – the shorter the wavelength, the higher the photon energy and the closer it comes to the band gap of the coating materials.

In the ultraviolet, photon energy approaches the band gap of common high-index oxides, and impurities, defects and band-tail states start to absorb. UV light can also create new absorbing defects over time, so stability under exposure matters as much as the initial value. That is why UV coatings rely on wide-band gap materials and extremely clean deposition.

The near-infrared is where dielectric coatings perform best. Photon energy is far below the band gap, so intrinsic absorption is negligible and only impurities and defects remain. Dense, amorphous IBS layers made from ultra-high-purity materials keep these to a minimum – critical for multi-kilowatt CW and high-average-power ultrafast lasers, where the absorbed heat grows in direct proportion to laser power.

The type of optic matters too. In an HR mirror, light reaches only the top layers of the coating, while in AR coatings and the transmitted polarization of a polarizer it passes through the whole stack. For femtosecond and picosecond lasers, high peak intensity adds nonlinear absorption – strongest in the UV.

Disclaimer

Absorption values were measured by LIDARIS using photothermal common-path interferometry (PCI), following the same standardized procedure for every sample, on a single coated surface. In PCI, a pump laser at the test wavelength heats the coating slightly, and a low-power probe beam detects the resulting thermal lens. The signal is proportional to the absorbed power, so absorption can be resolved down to sub-ppm levels.


Each sample is evaluated with three complementary scans:


Longitudinal scan (L-scan)
– the measurement point is moved through the thickness of the optic, from the front surface to the rear surface. Absorption shows up as sharp peaks at each surface, while a raised baseline between them indicates bulk absorption in the substrate. This separates coating absorption from substrate absorption.


Time scan
– the beams are held on one spot of the coated surface for about 11 minutes. This shows whether absorption is stable under continuous irradiation, or whether it drifts as the coating heats up or conditions.


Transverse scan (T-scan)
– the measurement point is moved 3 mm across the coated surface. This shows how uniform absorption is across the coating and reveals any local defects or contamination. The reported absorption value is the median of this scan. The uncertainty is the spread of values with statistical outliers removed, so a single defect does not distort the result.