My problem may not be very general. Imagine you observe the sun through thick clouds in multiple wavelengths. Given the spectrum of light starting off the sun's surface, you can calculate how rays will scatter, be absorbed and re-emit passing through the cloud given the 3d distribution, mass, and chemical composition of water vapors.

I want to do similar thing with my hydrodynamical galaxy simulation data. Classically, we've done this by following rays and it is time consuming. I believe if I need it scientifically accurate, I will have to solve the equations forward.

But, just for the visualization purpose, would there be a way to get rough synthetic images given 3d position and properties of light sources, scattering and absorbing material?

I am not an ML expert. So, I want to know if this exercise will worth anything before I start.

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