Since we're getting into the regime of higher power operations, we need to start thinking about TCS from a higher-order mode standpoint (higher than just spherical power/defocus). The current CO2 laser central heating and the ring heater provide almost 100% spherical power correction to the optic. The SELF heating, however, still produces a partly non-spherical lens from the absorption of the Gaussian beam.
These residual non-spherical lenses will increasingly cause problems as we go to higher power.
I've run a quick analysis of how much TEM00 is scattered AFTER the nominal spherical lens is corrected. This is purely for the substrate thermal lens (not for surface deformation, which is about 1/12th of the size).
For this model:
The scatter is calculated in the following way:
w0 = 54E-3;
k = 2*pi/1064E-9;
E1 = exp(-(r/w0)^2)
OPD1 = uncompensated lens (dobule-passed)
S0 = best fit defocus (spherical power) to uncompensated lens
OPD2 = OPD1 - S0/2 * r^2 % the residual thermal lens after spherical power is removed
E2 = E1*exp(i*k*OPD2)
OL = sum(r*conj(E1)*E2)*sum(r*E1*conj(E2)) / [ sum(r*E2*conj(E2))*sum(r*conj(E1)*E1) ] % overlap between pure gaussian and gaussian with residual thermal lens added as phase front error
scatter = 1- OL
The resulting plot shows the fractional scatter versus the absorbed power.
For reference, we'd really like to keep the round-trip scatter to 0.1% or less. The next step should be reviewing a detailed SIS model to try to refine these numbers.
Conclusion: we should consider a more appropriate CO2 heating beam shape for O2B.