The figure below shows the ablation window depth as a function of stage scan speed. The removal rate shows exponential decay, but the obvious fact points towed lower removal rates at lower energies; what's important is that the user can still control how stuff is removed by laser.
Fig. 1 shown below, shows signs of a minimum window depth feasible within any pulse energy given the maximum scanning speed available. The most important curve is the seemingly flat 35 µJ pulse energy profile, (1 µJ = 10-6J) which stays flat no matter the scan speed, as seen above. The other two energies (167 and 73 µJ) show clear decay slopes, which can be interpreted as progressive erosion by sample speed reduction (going backwards on the x-axis in Fig. 1 above). The calibration profiles on the left conform to this finding.
Figs 2-4 are scanning electron microscope (SEM) micrographs, AKA, closeups, of the coating after different laser energies. Fig. 2 is unabated; Fig. 3 depicts the coating after the 35 µJ laser; Fig. 4 is after 167 µJ. The coating itself is a TiO2 pigment (small white particles) embedded within the polyurethane binder (uniform dark background); the large spheres and blocky objects are siliceous and talc fillers, respectively.
The laser darkens the pigment to various degrees, even for the 35 µJ laser, which did not ablate the coating. The 167 µJ scan destroyed most of the pigment and considerably altered the binder morphology to the point of creating a large crater on the surface. Fig. 5 is a cross-section of the coating and shows a sharp distinction between the ablated and non-ablated regions.
band gap which makes it more susceptible to ablation than the surrounding polyurethane binder.
It's going to get a little technical from here on out, but this is where it gets quantitative. Fig. 6 shows the transmission spectra of a baseline (pristine) sample plus spectra from all three ablation energies (35, 73, 173 µJ).
The peaks contained within the box on the left did not change much after ablation; this is to be expected since polyurethane binder is mostly what's left in the ablated regions. There's a large gain in the peak on the right (indicates a gain in quantity for that functional group), but that's a region of considerable overlap between the C–O–C ether and O–Si–O; the authors guess it to be Si–O, since there's a lot of new SiO2 filler exposed.
Now I compare samples that differ by the amount of simulated weather that they've been exposed to. Below is Fig. 7.
Keep in mind that cm-1 (wavenumbers) is a unit of frequency just like Hz (s-1); in fact it's proportional by E = ℎν = ℎc/λ for the infrared radiation (IR). You could see from Fig. 7 that the IR is compared for the baseline, 6-weeks QUV exposed, and 18-weeks QUV exposed. The authors emphasize the complete extinction of the so-called amide II functional group, which means drastic decay for the polyurethane binder. In part (b) of Fig. 7, the OH/NH band broadens, perhaps due to carboxyl group formation. Simultaneously,the QUV process reduces the hydrocarbon peaks in the region close to 3000 cm-1.
Fig. 8 presents depth profiles of the ablated window for the baseline and 18-week QUV samples.
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Fig.1 Calibration profiles for three different energy levels at several scanning speeds (dwell times). Note absence of ablation window at 35 mJ energy level regardless of scan speed. |
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Fig.2 SEM micrograph showing surface detail of baseline (unablated) coating sample. |
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Fig.4 SEM micrograph showing surface detail of coating sample after 167 mJ ablation, 10K mm/s scan speed. |
band gap which makes it more susceptible to ablation than the surrounding polyurethane binder.
It's going to get a little technical from here on out, but this is where it gets quantitative. Fig. 6 shows the transmission spectra of a baseline (pristine) sample plus spectra from all three ablation energies (35, 73, 173 µJ).
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Fig. 6. Transmission-mode spectrum of unaged baseline and ATR-mode spectra for 35, 73 and 167 µJ ablation. The ester and urethane peaks experienced little change from the ablation process. |
Now I compare samples that differ by the amount of simulated weather that they've been exposed to. Below is Fig. 7.
Keep in mind that cm-1 (wavenumbers) is a unit of frequency just like Hz (s-1); in fact it's proportional by E = ℎν = ℎc/λ for the infrared radiation (IR). You could see from Fig. 7 that the IR is compared for the baseline, 6-weeks QUV exposed, and 18-weeks QUV exposed. The authors emphasize the complete extinction of the so-called amide II functional group, which means drastic decay for the polyurethane binder. In part (b) of Fig. 7, the OH/NH band broadens, perhaps due to carboxyl group formation. Simultaneously,the QUV process reduces the hydrocarbon peaks in the region close to 3000 cm-1.
Fig. 8 presents depth profiles of the ablated window for the baseline and 18-week QUV samples.
Fig. 10 shows FTIR depth-profile measurements. This is the nitty-gritty of the study, as it shows why this method falls short.
Fig. 11 a) repeats a result from an older study where they used transmission-mode FTIR on 3 µm thick cross-sections of the same two samples. It's mentioned here for the sake of comparison. Peak ratios are used here to eliminate fluctuating values due to varying sample thicknesses. Part (a) shows a clear change in the ratios as the depth is increased, meaning the near-surface region is more weather-damaged than the deeper regions in the bulk. That is not the case for part (b); if the ablation method did its job, it would show a damage gradient just like in part (a). The next blog will discuss why this is so.