Hello,
I have a question about POP analysis at a pixel grid. My system is defined by:
- a single F/7 lens with the shape of the James Webb Space Telescope (JWST) primary mirror
- a silicon substrate that contains the JWST lens focus inside it
- a MIRROR user-defined aperture aft the JWST lens focus. The user-defined aperture is a pixel grid with 25 micrometer wide square pixels and 2 micrometer wide gaps between the pixel.
- The propagated wavelength is 5.6 microns.
The problem I am facing is that, when propagating the wavefront back from the pixel grid (i.e. after the reflection on the pixels) to the JWST lens focal plane, the POP output shows a dark grid with zeros on the projected location of the pixel gaps. This is shown in the attached irradiance figure, where a dark grid is superimposed on the JWST PSF.
I have tried increasing the wavelength to 11 microns, thinking that the studied wavelength of 5.6 microns might be too small to interact with the pixel grid when propagating in silicon, but the issue remains. I have also tried increasing the sampling of the simulation, but this also doesn’t fix the issue.
Any help with this is appreciated. My expectation would be that the incoming wavefront should be convolved with the pixel grid pattern, rather than yield zeros at the location of the pixel gaps, but maybe I’m missing something.
Thank you in advance,
Yannis